text:
Night Queen Online Slot Review
iSoftBet released a new slot game, Night Queen. The slot game is based on the classic novel of the era and features some gothic and dark elements of the game. This is not the first time, the UK-based developer managed to surprise the customers with impressive graphics and vibrant design. Recently, the slot game developer released the very successful sequel Hot Shot 2.
Games by iSoftBet are very popular among the customers. The slot games are outstanding with the vibrant visuals, the great graphics, and of course some of the very unique features. The game developer is licensed in 17 different markets and thus is present in many online casinos all over the world. One of the online casinos, which can already offer the brand new slot to the customers is PlayAmo.
Night Queen Features
The slot game is extremely high volatility, meaning that if you are not up for risks, then you should not play this game at all. The riskier it gets, the more you can win, but the more you can lose as well. Some of the features prove the high volatility of the game. The Night Queen slot game comes with 5 reels, 3 rows, and 20 pay lines.
The high volatility game has a relevant RTP rate as well as high paying symbols. Some of the lowest paying symbols are the royals from 10 to A. There are some of the high paying symbols present in the game as well. Those symbols include the raven, stallion, mysterious gentleman, and the main character of the game who is the fair-eyed Night Queen, which is also the highest paying symbol of the game.
As mentioned before, some of the unique features are present during the gameplay. The first one that should be mentioned is the Switching Stacks mechanic. During the activation of this specific feature, the stacked symbols can switch with each other after every single spin. This is made in order to assist in generating the wins. If three or more reels of stacked winning symbols land, they should come together to form one mega symbol, which may then trigger the random win multiplier of up to 30x, which will apply to the total wins.
One more feature which is definitely worth mentioning is the bonus spins, which is one of the most exciting parts of every slot game. The bonus spins promise bonuses that are the cash rewards. The bonus spins round can be activated when three or more Night Queen symbols land on the reels. This is where Mystery Symbols always land stacked, which means that they are also able to get into Switching Stack mode. The symbols will also be revealed after the spins at the end of the switching. This is what made the fantastic Super Stacks on the reel, generate even more and even bigger wins.
After the release of the game, the official representative, Mark Claxton of iSoftBet company made an announcement. After the announcement of the release of the new game, he made a statement, stating that the Night Queen game can be considered as one of the most unique products. This can be proved by the fact that the Night Queen slot game combines the land-based gameplay feeling, which can be experienced only in land-based casinos, and together with that it also combines the ghoulish, haunting theme, taken away from the classic novel.
The Night Queen is a must-try slot game if you are at least in favor of high volatility games and enjoy taking risks. It offers a lot of opportunities that come along in the gameplay. Some of the symbols and features present in the game, can trigger huge multipliers and thus generate colossal wins, which is the best reward in the slot game.
The main thing to consider is that, despite the high volatility, the slot game manages to support the whole gameplay and make it more and more exciting during the whole process. This is one of the most important parts of the gameplay. You can never get tired, and must always expect something better and bigger to come your way.


text:
Particle Acceleration in three dimensional Reconnection Regions: A New Test Particle Approach
Magnetic Reconnection is an efficient and fast acceleration mechanism by means of direct electric field acceleration parallel to the magnetic field. Thus, acceleration of particles in reconnection regions is a very important topic in plasma astrophysics. This paper shows that the conventional analytical models and numerical test particle investigations can be misleading concerning the energy distribution of the accelerated particles, since they oversimplify the electric field structure by the assumption that the field is homogeneous. These investigations of the acceleration of charged test particles are extended by considering three-dimensional field configurations characterized by localized field-aligned electric fields. Moreover, effects of radiative losses are discussed. The comparison between homogeneous and inhomogeneous electric field acceleration in reconnection regions shows dramatic differences concerning both, the maximum particle energy and the form of the energy distribution.
PACS numbers: 52.20 ; 52.65.C ; D95.30 ; 95.30Q
I Introduction
The acceleration of charged particles in space and astrophysical plasmas is a matter of debate in contemporary plasma astrophysics (cf. reviews [1] and [2]). Beside the "standard" acceleration mechanisms as shock waves ([3], [4]), Fermi acceleration [5], and magnetic turbulence ([6], [7]) acceleration by magnetic field-aligned electric fields receives more and more attention as it offers the capability for efficient and fast energization of relativistic particles ([8], [9]). The formation and amplification of such electric fields in the context of magnetic reconnection processes has been discussed for different cosmical plasmas and parameter regimes ( [10], [9], [11], [12], [13]). Since magnetic reconnection can be regarded as an unavoidable dissipation and relaxation process in magnetized plasmas under the influence of externally driven shear motions, the principal importance of magnetic reconnection electric fields is now widely accepted.
Analytical and numerical studies have significantly improved our understanding of energetic particle trajectories in reconnection configurations without ([14], [15], [16], [17], [18], [19]) and with ([20], [21], [22]) a magnetic field component parallel to the reconnection current sheet. Nevertheless, the particle trajectories and, in particular, the actual energy gains of accelerated charged particles in the reconnection current sheets prove to be still a crucial matter of debate, since the studies mentioned above have been performed for idealized analytical electric and magnetic field configurations which differ significantly from the three-dimensional configurations characterized by localized field-aligned electric fields as observed, e.g. in the solar corona (cf. [23]) and the Earth's magnetosphere (cf. [24]). Test particle simulations of ion ([25]) and electron ([26]) injection in a high-beta magnetospheric substorm configurations have shown that the consideration of more complicated 3d field configurations rather than idealized 2D ones is crucial for the understanding of particle acceleration in reconnection regions. In this contribution we study the acceleration of charged particles up to relativistic energies in reconnection regions. The electromagnetic fields of the reconnection region are modeled by 3D-magnetohydrodynamic (MHD) simulations of a reconnection zone in a current carrying magnetic flux tube. Since the astrophysical evidence for the existence of relativistic particles relies only on the electromagnetic radiation emitted by of these particles, we calculate the motion of high-energy particles by means of relativistic test particle simulations including radiative forces due to inverse Compton scattering and synchrotron radiation. We consider our study as a step forward to a self-consistent description of particle acceleration in quite realistic reconnection configurations.
The manuscript is organized as follows: The next section presents the motivation for our new approach. Sec. III describes the electromagnetic field configuration we used and how they are obtained from MHD simulations. These fields represent the external force field, to be supplemented by radiative forces, for the relativistic test particle calculations, described in Sec. IV. The results of these test particle simulations are compared with the analytical and numerical X-type configuration of the reconnection magnetic field in Sec. V. Sec. VI is devoted to a discussion of our results.
Ii Motivation for our new Approach
Particle acceleration in magnetic reconnection zones has been extensively discussed and studied analytically and numerically (we refer to the analytical papers [14], [27], [28], [22], and references therein); numerical treatments can be found in [16], [29], and references therein). These investigations rely on one common assumption The homogeneity of the electric field. The authors have used an analytical formulation of the electric field configuration and therefore the calculations are highly idealized. The field configurations found in the papers mentioned above are nearly identical and can be written as
The process of reconnection in two dimensions is still subject of intense scientific investigation up to the present day. Besides first analytical approaches ([30]; [31]) investigations of the much more complex 3D reconnection process are restricted to numerical modeling. In a 2D description the X–point configuration
that describes a hyperbolic magnetic field with a neutral line in the center (), has become the standard model of reconnection. With Amp re's Law
Ohm's Law
and invariance in one dimension, say , one can easily derive the electric field
If one assumes a constant resistivity and that the convective term is small as compared to the first term in (Equ. 5) in the localized reconnection zone the constant, homogeneous, infinitely extended electric field is given by
Such an electric field is, without question, unphysical. In case of a 2D reconnection calculation this is not a severe problem, because the electric field is never used as a real physical quantity. For this reason one can argue that it is merely a mathematical auxiliary variable and only the magnetic field is needed to describe the complete electromagnetic configuration.
However, this X–type field is a valid approximation of the inner part of a reconnection region around the neutral line. Only the application of this idealized configuration in the context of particle acceleration gives rise to serious problems. The electric field is the source of energy for the accelerated particles and exactly this very reason for acceleration is, as stated above, unphysical. At this point, we should ask how sensible are the results concerning particle energy spectra, duration of acceleration etc., derived from an idealized, homogeneous electrical field? For example, there are particle trajectories
for which particles will gain infinite energy. This comes from the fact that the electric field lacks any dependence on the invariant direction.
In order to accelerate particles efficiently a strong guiding component ([27]) is needed. With such a strong component the magnetic field is almost parallel to the electric field in a region around the neutral line. In addition, this guiding component captures the particles in the zone, at least as long as their gyroradius is smaller than the width of the reconnection zone. These two facts guarantee the efficient acceleration described in [27]. On the other hand this configuration in the center of a X field with strong resembles remarkably that of a simple capacitor. Any particle following the field lines is accelerated exactly linear, like in a capacitor. The energy gained by such a particle is directly given by
denotes the energy gain and is the charge of the particle that is accelerated along the magnetic field line over the distance .
The energy gain does not depend on the detail of the reconnection process, but on the geometry of the acceleration region only.
Moreover, one has to take into account the convective electric field components and , which are completely neglected by most authors, though they naturally arise in realistic descriptions of reconnection zones. Such fields are generated by external shear flows which are the macroscopic generator of electromagnetic energy converted partly into particle kinetic energy in the localized dissipative reconnection zones. Calculations with three-dimensional magnetohydrodynamic (3D-MHD) codes clearly show (e.g. [32]) that those components are often much stronger than the field line parallel electric field . The precise influence of those components is not known, nevertheless we should not neglect them strait from the beginning, without knowing anything about the strength of their influence. We speculate that such convective electric fields can filter out particles from an efficient acceleration due to their strength and structure and dependent on the initial positions of the particles. In other words, the form of the energy distribution may be closely connected to these electric fields.
The above questions convinced us to approach again this well known and well studied phenomenon of particle acceleration in magnetic reconnection zones. Contrary to other investigations, we use a field configuration, which is produced with the help of a full 3D-MHD code.
Iii The 3D-MHD Simulations of Magnetic Reconnection
The MHD framework for the particle simulations of electron acceleration in reconnection regions is built up by means of a three-dimensional MHD code [33]. It is motivated by previous works on reconnection in the context of planetary magnetosphere-ionosphere coupling ([11], [13], [22], [32], [34]) and of active galactic nuclei [12]. However, the situation we have in mind (cf. Fig. 1) is quite general and may be regarded as a rather generic reconnection configuration that arises when MHD shear flows working as electromagnetic generators sheared magnetic fields. For convenience, we start from a two-dimensional force-free magnetic field
We choose for the constant main component and the shear component of the magnetic field and in normalized units. The plasma is chosen to be isothermal as well as homogeneous, initially. We note that, alternatively, an appropriate equilibrium that includes thermal pressure forces could be realized. This ideal equilibrium is perturbed by
As a boundary condition for we use
These velocity perturbation with an amplitude chosen as of the Alfvén velocity mimics some external convective plasma motion which leads to a further shear of the magnetic field and an increase of the field-aligned current density. The associated magnetic perturbation is transported along the -component of magnetic field via shear Alfvén waves. Here, we follow the general concept that plasma systems that are compelled by such external forces when some critical parameter(s) is (are) exceeded non-linearly develop into a state of lower energy thereby releasing stored free energy in form of dissipative plasma heating and particle acceleration.
In the considered configuration the magnetic field-aligned current density plays the role of the critical parameter. When the current density exceeds a critical value (we choose a marginal current density at the beginning) a current dependent resistivity, which is localized in the - and -direction is switched on. This violation of ideal Ohm's law starts the magnetic reconnection process (cf.[9]). Fortunately, for our purpose we have not to dwell on the specific nature of the finite resistivity, may it be microturbulent [35] dissipation or particle inertia [36] or whatever. For the MHD simulations we choose the following technical details:
The dimensions of the numerical box are given by , , and in normalized units. We make use of line symmetry as a boundary conditions at , i.e. the - and -components of the magnetic field and the velocities are chosen antisymmetric whereas the -components of these quantities are chosen symmetric about . Boundary conditions in are chosen as symmetric and in as well as at we use extrapolation. The simulations are carried out with grid points in the - direction, grid points in the -direction and grid point in the -direction.
The numerical grid is a non-uniform one with a maximum resolution of in the -direction, in the -direction, and in the -direction.
Some characteristic fieldlines are shown in Fig. 2 to give an idea of the overall structure of the magnetic field. In Figs. 3 to 6 we show the Cartesian components of the electric and magnetic fields which are chosen as an input for the particle simulation studies. The figures show the fields after where is the characteristic Alfvén velocity of the system. At this state of the temporal evolution the reconnection process can be considered as quasi-stationary, i.e. the magnetic flux is as rapidly piled up by the shear flow as it is annihilated by
magnetic reconnection.
The -component of the magnetic field results from the shear flow and from the divergent reconnection flow (Fig. 3, top panel) and (Fig. 4, top panel). The -component of the magnetic field (middle panels of Fig. 3 and Fig. 3) is associated with the current sheet and modified by reconnection convergent flows (). The -component (lower panels of Fig. 3 and Fig. 3) shows a rather moderate variation due to the reconnection process. The three-dimensional electric vector field at the height of the central reconnection region is illustrated in Fig. 5. The convective -component (top panels of Fig. 5 and Fig. 6) is the result of both the applied sheared flow and the divergent reconnection flow whereas the convective -component (middle panels of Fig. 5 and Fig. 6) is due to the convergent reconnection flow. The convective electric fields are about one order of magnitude higher than the -component of the electric field (lower panels of Fig. 5 and Fig. 6) which is caused by the finite anomalous electric resistivity . is localized in the - and -direction (we have chosen for the resistivity profile ) and is most important for the acceleration of charged particles.
It is mainly responsible for the non-vanishing elongated generalized field-aligned electric potential ([9], [37]) (where the integration is extended over the arch length ). Such potentials are observed, e.g. as "auroral potential structures" in the Earth's magnetosphere [38] which are responsible for the acceleration of auroral electrons. The three-dimensional electric and magnetic vector field are used as an input for the test particle simulation studies of relativistic electrons as discussed in the next chapter. Note, that these rather complex fields, which are due to shear Alfvén waves, shear motion and reconnection dynamics, differ significantly from idealized configurations usually discussed in the literature. We consider the electromagnetic field shown as a quite typical reconnection configuration in systems that are characterized by shear flows. Since it represents the self-consistent reconnection dynamics it can be qualified as a realistic configuration in comparison to idealized two-dimensional ones.
Iv Particle Acceleration
We use the fields described in Sec. III for electron acceleration. By means of a fully relativistic test particle code, including energy losses due to synchrotron emission (SY) and inverse Compton scattering (IC) we analyze the fate of the relativistic particles. The term "test particle" in this context means that any back-reaction of particles on the electromagnetic field configuration is neglected. As long as only a fraction of particles is actually accelerated, i.e. as long as the particles leave the acceleration zone on time scales much shorter than the Alfvénic time this is a very good approximation, which is always fulfilled during our simulations, since the particles are efficiently accelerated along the magnetic field line and move with almost the velocity of light. Moreover, no interaction between the particles is included.
For the integration of the relativistic equations of motion
we use the classical fourth order Runge-Kutta algorithm together with an adaptive stepsize control [39]. Our 3D-MHD fields are only known on a discrete 3D grid. For this reason, we have to interpolate these fields for positions in between by means of a simple linear interpolation algorithm.
As described in Sec. III the electromagnetic fields can be regarded as quasi-stationary after some hundred Alfv nic times . Moreover, the test electrons are accelerated on a very short time scale (cf. [40]). For this reason there is no need to consider the precise dynamic evolution of the MHD fields. We can use them as static background fields without any temporal changes and this is also a very good approximation. In addition to the Lorentz force our code considers the complete loss force [41]
where , , and denote the charge, the mass, the velocity and the Lorentz factor of a particle, respectively. This loss force describes all particle-field interactions, inclusive synchrotron radiation (SY) and inverse Compton scattering (IC). SY presents the radiation of relativistic electrons, gyrating around the magnetic field, i.e. it influences the particle momentum perpendicular to the magnetic field. If an acceleration process injects particles merely along the field lines these particles undergo no synchrotron losses. However, since we inject particles isotropically from all directions, the particles will have finite pitch angles at the beginning. Even for very anisotropic energy distributions in the sense that the particles move only parallel to the magnetic field lines particles may suffer radiative losses caused by inverse Compton scattering, if an intense photon bath is present in the environment of the acceleration zone. The radiation mechanisms depend on the energy of the particles and the energy density of the magnetic field (SY) or the photons (IC), respectively,
Qualitatively, it is clear that relatively strong (in terms of efficiency and short time scales) particle acceleration via magnetic reconnection requires significant magnetic field strengths. Since astrophysical plasmas are highly conducting media, strong magnetic fields are related with either fast plasma motions or high plasma pressure and temperature, i.e intense radiation fields. Such conditions are typical, e.g., for compact astrophysical objects, as neutron stars or black holes and magnetospheres of young stellar objects. Often the magnetic field energy density and the radiation energy density are of comparable order, or at least proportional to each other. This quality is again connected with the high electric conductivities of astrophysical plasmas on macroscopic spatial scales. If plasma is accelerated due to some radiation pressure, the magnetic field is strongly coupled to the plasma motion and is amplified by field line compression and twisting. The plasma temperature is directly related to the radiation temperature. Thus, a significant variation of the emitted radiation will consequently produce varying plasma temperatures and pressures, which finally leads to magnetic field amplification (e.g. [42]). Thus, the energy losses of the accelerated particles can be handled by a simple scaling .
V Comparison
We use our code for the calculation of electron energy spectra which one would expect to be the final energy distributions in some selected configuration. In order to perform this we calculate the trajectories of more than 8000 electrons, which start at random places with a random momentum and determine their final energies, when they leave the numerical bounding box of the MHD fields. The initial positions are equally distributed in the whole reconnection region. The initial momentum of the electrons is chosen isotropic with absolute values that correspond to a Maxwellian distribution of the initial energy.
In Fig. 7 the initial energy distribution of the electrons is shown. Here and in all following plots "Relative Frequency" is the normed () percentage of particles per energy interval. All runs start from this distribution. Fig. 8 shows the final energy distribution of electrons accelerated in our quite realistic 3D-MHD fields (see Sec. III). Most electrons are accelerated due to the strong guiding component . Energies in the range from to nearly are seen. One first remarkable fact is the existence of electrons nearly without any energy gain. A second interesting feature is the obvious depression in the middle of this spectrum.
It seems as if there exists some sort of selection process, which does not allow a particle to achieve an energy between and . This might indicate that there are unstable trajectories, which lead exactly to this energy range. The high energetic end of the particle distribution is determined by the thickness of the resistive region. Only in the region of finite resistivity a parallel electric field is present, which can accelerate the particles efficiently.
The gyro radius of an accelerated electron is given by
which depends on the energy of the electrons ( is the thermal velocity of the electrons). Particles are accelerated, in the best case, as long as their gyro radii are smaller than the extent of the resistive region. This criterion gives the maximum energy gain achievable. The effect of considering the loss force (Equ. 13) is shown in Fig. 9. In order to illustrate those effects we overestimate the strength of the loss force by assuming an extremely
intense photon bath with an energy density of about ten times the maximum magnetic energy density . Very few electrons are now able to achieve more than . This is the energy, where the loss of energy due to radiative processes balances the energy gain from the electric field. The characteristic features mentioned before remain unchanged apart from the new upper limit for the final energy, which leads to a "pile-up" at about .
After all, it can be stated that the usage of rather realistic 3D-MHD fields, i.e. a field configuration that represent evolved reconnection electromagnetic fields rather than analytical idealized fields, gives a rich spectrum displaying a great variety of features. This changes drastically in the case of an oversimplified homogeneous electric field. The next example is calculated with the electric field
where denotes the maximum of the component of the numerical electric field used before. The resulting energy distribution, calculated in the same way as before, is shown in Fig. 10. We should point out that for this simulation nothing has been changed in the magnetic field configuration. Fig. 10 shows a very narrow spectrum around the energy completely without any feature so characteristic for the spectrum of Fig. 8. First of all, we can clearly see that every electron is accelerated. This unphysical result comes at no surprise, because a constant electric field in combination with the strong guiding component implies an infinite resistive region. The obvious absence of any structure shows, that the origin of the depression has to lay mainly in the electric field. An oversimplification of neglects this interesting effect. The enlargement of the resistive region to the whole numerical box also erases the upper limit of acceleration. The maximum energy is given by the potential difference between on side of the box and the other, but that is a pure trivial geometric limit.
In addition, there is no similarity between the rather realistic spectrum Fig. 8 and that calculated with a homogeneous electric field Fig. 10.
Comparison of the pitch angle distribution (Fig. 11) of the realistic simulation with the one of the oversimplified electric field simulation (Fig. 12) also shows a striking difference. While both distributions clearly show that a vast majority of electrons is moving mainly along the magnetic field lines, again a broad spectrum over tree decades and a small amount of electrons, which have a pitch angle greater than evolves (Fig. 11). The pitch angle distribution in Fig. 12 on the other side is lacking any hint of the electron population with an pitch angle greater than . An homogeneous electric field can, in fact, not be regarded as a valid approximation of a realistic field configuration.
At this point the question arises, how important is the structure of the magnetic field for the final spectra anyway? In order to answer this question we finally consider the spectrum for
This spectrum (Fig. 13) shows a striking similarity with the previously shown one Fig. 10. Both spectra are dominated by the geometry of the numerical box. All of the features seen in Fig. 8 are coming from the complicated structure of the electric field. It seems that the structure of the magnetic field serves only as "stage" for the electrons without significant influence on the spectra. Nevertheless, we should keep in mind, that the field determines the structure of the field.
Vi Discussion
Astrophysical plasmas like the interstellar or intergalactic medium and compact systems like accreting stellar objects are magnetized and highly conducting collisionless media under the influence of external forces. The main driving forces for plasma-magnetic field motions are gravity, rotation and pressure gradients. Due to the lack of significant particle collisions astrophysical plasmas are easily forced to steep magnetic field gradients, which ultimately will evolve into relaxed field configurations via magnetic reconnection. In that sense magnetic reconnection is an unavoidable result of external distortions in collisionless magnetized plasmas. The important observable consequences of reconnection for astrophysical applications follows from the fact that it accounts for heating and particle acceleration by locally converting the stored magnetic energy into bulk heating of the plasma via Ohmic heating or acceleration of a population of high energy particles via magnetic field-aligned electric fields that are associated with the finite conductivity.
The heating capabilities of magnetic reconnection have been investigated in detail, since the heating rate is a macroscopic quantity which depends only on the density and temperature, but not on the details of the single particle response to the electromagnetic configuration inside a reconnection zone. In that sense it behaves like a macroscopic transport property.
The acceleration of particles instead depends on the local properties of the reconnection region. The energization of a charged particle above all depends on the effective electric force the particle "feels". Depending on its initial position and initial energy the particle energy gain differs. Since the only source of information of high energy astrophysics is the electromagnetic radiation, the energy distribution of relativistic particles is one of the most required issues concerning the interpretation of nonthermal radiation sources. Thus, for any acceleration process discussed it is most important to investigate the resulting energy distribution functions in dependence on the various parameters on which the acceleration process depends on. In this context, the two-dimensional models published so far for the acceleration of charged particles by magnetic reconnection are not satisfying, since they describe acceleration in linear conductors. They do not describe the effect of the finite extension of the acceleration zone and show always a purely monoenergetic distribution at the maximum energy the particles are "allowed" to reach. The maximum energy in these models is simply given by the product of the homogeneous electric field times the chosen length of the reconnection zone, which is supposed to be a free parameter. This is definitely incorrect; the system size must be finite and must depend on the process responsible for the violation of ideal conductivity.
We have shown the pitfalls of the two-dimensional ansatz and present 3D-simulations of MHD-reconnection plus test particle simulations within the MHD-frame, including radiation losses (synchrotron and inverse Compton scattering). The precise structure of the electric field is the determining factor of the acceleration process in the MHD reconnection region (cf. Sec. V). One has to be extremely careful in simplifying the electric field; in our example the spectrum calculated with a homogeneous electric field is no good approximation to the one that results from a physically motivated field.
Since the investigated magnetic field configuration is a valid 3D generalization of a 2D X-type field the usage of an homogeneous electric fields in X-type electric fields should also be misleading as far as the spectrum is concerned.
Whereas particle acceleration in a simplified X-type configuration with a homogeneous electric field is an interesting subject of it's own, it is obviously not appropriate for the study of particle acceleration in magnetic reconnection zones. We have shown that for this task we need much more realistic fields and at least numerical approaches in future should use 3D-MHD fields. A further extension of the work presented in this contribution will be the consideration of multiple X-line and O-point reconnection configurations (c.f. [19] and [43] for the 2D case) which should show a larger class of different kinds of particles populations.
The strong influence of radiative losses on the resulting energy distribution of the accelerated charged particles, even without overestimation of the photon density, gives us the clear indication that we should not restrict ourselves to the use of realistic field configurations alone. By not taking into account SY and/or IC losses in relativistic particle acceleration processes in reconnection zones the particle pile-up at the upper energy limit is completely neglected and the maximum energy of the particles is incorrectly estimated. This shows that the consideration of loss processes should be obligatory for the determination of quantitative results in the relativistic case. In this context we briefly note that particle acceleration by 3D-reconnection has considerable observational consequences. As is obvious from our simulations 3D-reconnection produces power-law energy distributions, which would emit power-law radiation spectra, i.e. decreasing radiation flux with increasing frequency : Flux . For synchrotron and inverse Compton emission the index of the energy distribution is related with the spectral index via In contrast the simple analytical models with a constant electric field give mononergetic energy distributions which give synchrotron spectra where the received radiation flux increases with increasing frequency up to some critical frequency determined by the energy of the accelerated particles (Flux for an optically thin monoenergetic source) (c.f. [44]).
At the present time we do not consider any interaction between particles and plasma waves and we neglect losses due to pair production. These effect should be addressed in future simulation studies as well as the interplay of second order magnetic fields induced by accelerated particle beams and the ponderomotive force of the excited plasma fluctuations. We feel that such studies will prove to be very helpful to clarify the role of reconnection in a variety of dynamical astrophysical plasma phenomena as different as, e.g., extragalactic jets, TeV burst and solar flares.
This work was supported by the Deutscher Akademischer Austausch Dienst (DAAD) through the grant D/98/02999, the Alexander von Humboldt foundation through the Feodor Lynen program (GTB) and the Deutsche Forschungsgemeinschaft through the Schwerpunkt "Physik der Sternentstehung" and the grant Le 1939-4/1.
- [1] J.G. Kirk, Plasma Astrophysics (Springer, Berlin, 1994) p. 225.
- [2] J. Kuijpers, Lect. Notes Phys. 469, 101 (1996).
- [3] V.L. Ginzburg and S.I. Syrovatskii, The Origin of Cosmic Rays (Pergamon Press, Oxford, 1964).
- [4] R.D. Blandford and J.P. Ostriker, Astrophys. J. 221, L29 (1978).
- [5] E. Fermi, Phys. Rev. Lett. 75, 1169 (1949).
- [6] R. Ramaty and R.J. Murphy, Space Sci. Rev. 45, 213 (1987).
- [7] R. Schlickeiser, Astrophys. J. 336, 264 (1989).
- [8] H. Alfvén, Cosmic Plasma, (Reidel, Dordrecht, 1981).
- [9] K. Schindler, M. Hesse, and J. Birn, Astrophys. J. 380, 293 (1991).
- [10] E.R. Priest, Solar Magnetohydrodynamics, (Reidel, Dordrecht, 1987).
- [11] A. Otto and G.T. Birk, Geophys. Res. Lett. 20, 2833 (1993).
- [12] H. Lesch and G.T. Birk, Astron. Astrophys. 324, 461 (1997).
- [13] A. Kopp, G.T. Birk, and A. Otto, Planet. Space Sci. 46, 405 (1998).
- [14] T.W. Speiser, J. Geophys. Res. 70, 4219 (1965).
- [15] S.W.H. Cowley, Planet. Space Sci. 27, 539 (1978).
- [16] H.-J. Deeg, J.E. Borovsky, and N. Duric, Phys. Plasmas B 3, 2660 (1991).
- [17] R.W. Moses, J.M. Finn, and K.M. Ling, J. Geophys. Res. 98, 4013 (1993).
- [18] G.E. Vekstein and E.R. Priest, Phys. Plasmas 2, 3169 (1995).
- [19] B. Kliem, J. Schumacher, and D.R. Shklyar, Adv. Space. Res. 21, 563 (1998).
- [20] Y.E. Litvinenko and B.V. Somov, Sol. Phys. 146, 127 (1993).
- [21] R.L. Kaufmann, C. Lu, and D.J. Larson, J. Geophys. Res. 99, 11277 (1994).
- [22] Y. Litvinenko, Astrophys. J. 462, 997 (1996).
- [23] R.D.Bentley and J.T. Mariska, Magnetic Reconnection in the Solar Atmosphere, Conference Series Volume 111 (Astronomical Society of the Pacific, San Francisco1, 1997)
- [24] Akasofu, S.-I. and J.R. Kan, Physics of Auroral Arc Formation, (American Geophysical Union, Washington, 1981).
- [25] J. Birn, M.F. Thomsen, J.E. Borovsky, G.D. Reeves, D.J. McComas and R.D. Belian, J. Geophys. Res. 102, 2325 (1997).
- [26] J. Birn, M.F. Thomsen, J.E. Borovsky, G.D. Reeves, D.J. McComas and R.D. Belian, J. Geophys. Res. 103, 9235 (1998).
- [27] S.V. Bulanov and P.V. Sasorov, Sov. Astron. Let., 19, pp. 464–468, (1975).
- [28] S.V. Bulanov, Sov. Astron. Let. 6, pp. 206–208, (1980).
- [29] M.V. Nocera, F. Pegoraro, S.V. Bulanov, and G. Bertin, Physica Scripta, T63, pp. 197–202, (1996).
- [30] P. Démoulin, J.C., Hénous, E.R. Priest and C.H. Mandrini, Astron. Astrophys. 308, 643 (1996).
- [31] G. Hornig and L. Rastätter, Phys. Scripta T74, 34 (1998).
- [32] G.T. Birk and A. Otto, J. Atm. Sol.-Terr. Phys. 59, 835 (1997).
- [33] A. Otto, Comp. Phys. Com. 59, 185 (1990).
- [34] G.T. Birk and A. Otto, Adv. Space Res.20, 1301 (1997).
- [35] J.D. Huba, Unstable Current Systems and Plasma Instabilities in Astrophysics (Dordrecht, Reidel, 1985), p. 315.
- [36] V.M. Vasyliunas, Rev. Geophy. Space. Phys. 13, 303 (1975).
- [37] K. Schindler, M. Hese, and J. Birn, J. Geophys. Res., 93, 5547 (1988).
- [38] F.S. Mozer, Physics of Auroral Arc Formation (American Geophysical Union, Washington, D.C., 1981), pp. 136–142.
- [39] W.H. Press, B.P. Flannery, S.A. Teukolsky, and W.T. Vetterling, NUMERICAL RECIPES in C (Cambridge University Press, Cambridge UK, 1988).
- [40] R. Schopper, H. Lesch, and G.T. Birk, Astron. Astrophys., 335, pp. 26–32 (1998).
- [41] L.D. Landau, E.M. Lifshitz, The Classical Theory of Fields (Addison–Wesley Publ. Comp., Reading Mass. USA, 1951).
- [42] R.D. Blandford, In Active Galactic Nuclei, Saas-Fee Advanced Course 20, (Springer, Heidelberg, 1990), p. 161.
- [43] J. Schumacher and B. Kliem, Phys. Plasmas 3, 4703 (1996).
- [44] M.S. Longair, High energy astrophysics (Cambridge University Press, Cambridge UK, 1981).

subset: commoncrawl


text:
Google finds security flaws in Apple's web browser: FT
Google researchers have found multiple security flaws in Apple's Safari web browser that allowed the tracking of users' browsing behavior, the Financial Times reported on Wednesday, citing a soon-to-be published paper.
The vulnerabilities were found in a tool specifically designed to protect privacy and could have allowed third parties to obtain sensitive information about the browsing habits of users, the report said.
Google disclosed the flaws to Apple last August, according to the report. In a blog post in December, an Apple engineer said the company had fixed flaws disclosed to it by Google researchers.
An Apple spokesman on Wednesday confirmed that the flaws found by Google and highlighted in the Financial Times' story were patched last year. Reuters
-- Contact us at [email protected]
On three misconceptions about the LGBTQIA+ community Brian YS WongThe District Council's collective decision of endorsing the Pride Parade (as part of the wider Pride Month celebrations of LGBTQIA+ diversity) has drawn substantial ire from many, with conservative
Another option for HK SMEs seeking govt support to digitise Kevin FitzgeraldThe Hong Kong Government's D-Biz Programme has been highly sought after as businesses now understand the importance of taking innovative, digital approaches to keep things up and running during the
End of Hong Kong as we know it Michael ChuganiOn a stormy morning on July 1 1997 I awoke with a heavy heart mixed with hope. Just hours earlier, at the stroke of midnight, the city where I was born had passed from colonial to communist rule.
A big PR deal Hong Kong doesn't need Ben KwokFinally, Chief Executive Carrie Lam Cheng Yuet-ngor was able to secure the services of a public relations firm to help rebuild the city's shattered international image. You will recall that her
Beijing's best shot - we are as vile as you Stephen VinesIf your best argument is not that what you are doing is right but that what others do is even worse, it is safe to conclude that you have a problem. Yet here we are as Beijing furiously mobilises all
End of Hong Kong as we know it
A big PR deal Hong Kong doesn't need
Saved by the Pandemic?
Why Indonesia is the next digital payments battleground
Coronavirus turns Boris Johnson's honeymoon into nightmare
The recovery plan America needs
On three misconceptions about the LGBTQIA+ community
SHOPLINE: "We are hiring, a lot."
Another option for HK SMEs seeking govt support to digitise


text:
Workaholics - Season 5 (2015) TV Show Online Free - 123 Movies
Watch Workaholics - Season 5 Full Tv Show Online free in HD on 123 Movies,Season 5 opens withĀAlice askingĀAnders to assemble a team of co-workers and head over to a near by .... You are watching the serie Workaholics - Season 5 (2015) TV Show Online Free - 123 Movies belonging in the genere of Comedy with total duration of each episode 30 , broadcasting at 0123movie.ws. This show was first release in the Country of United States with IMDb rating of 8.2 in the year of 2015. This show is now available at 123 Movies in HD Quality.
Genre: Comedy
Production Country: United States
Rating: 8.2
Actors: Blake Anderson
Release: 2015
Runtime: 30
Quality: HD


text:
Trump's baffling virus suggestion
US President Donald Trump has suggested injecting people with bleach or alcohol to fight coronavirus.
Calls to poison control and emergency hotlines in a number of US states have spiked in the days since President Donald Trump mused about injecting disinfectant into the body to wipe out COVID-19.
He soon backtracked on his comments from Thursday, telling reporters he was "asking the question sarcastically" despite being seen straight-talking to his medical advisers.
On Monday, Mr Trump said he "can't imagine why" there had been an increase in calls.
"I can't imagine that," he said.
Asked whether he took responsibility at all for the rise, he replied: "No, I don't."
RELATED: Follow the latest coronavirus updates
Governor of Maryland Larry Hogan, a fellow Republican, said his state had been swamped with queries.
"We had hundreds of calls in our hotline here in Maryland about people asking about injecting or ingesting these disinfectants," he told CBS on Sunday.
"Which is, you know, hard to imagine that people thought that was serious.
"But what people actually were thinking about this was, (is) this something you could do to protect yourself?"
Now more than ever, it's critically important for leaders to focus on the facts. As I reiterated this morning on @FacetheNation, I remain committed to being transparent, keeping Marylanders fully informed, and making the necessary decisions to keep Marylanders safe. pic.twitter.com/kZ2bYrDMBe— Governor Larry Hogan (@GovLarryHogan) April 26, 2020
He said it was "always critically important" for a leader to release facts and to be open, honest and transparent.
"And I think it's critical that the President of the United States, when people are really scared and in the middle of this worldwide pandemic, that in these press conferences that we really get the facts out there," Gov. Hogan said.
Maryland Emergency Management Agency had to warn residents against consuming or administering disinfectant to the body.
Gov. Hogan said callers to the health department's emergency hotline asked "if it was right to ingest Clorox", a disinfecting bleach, or alcohol cleaning products.
"We had to put out that warning to make sure that people were not doing something like that, which would kill people," Gov. Hogan told MSNBC.
"I think when misinformation comes out, or you just say something that pops in your head, it does send a wrong message."
ALERT🚨: We have received several calls regarding questions about disinfectant use and #COVID19.— Maryland Emergency Management Agency (MDMEMA) (@MDMEMA) April 24, 2020
This is a reminder that under no circumstances should any disinfectant product be administered into the body through injection, ingestion or any other route.
RELATED: Trump says China will be held 'accountable'
Governor of Michigan, Gretchen Whitmer, a Democrat, said similar scenes had played out in her state.
"When the person with the most powerful position on the planet is encouraging people to think about disinfectants, whether it was serious or not, people listen," she told ABC News' This Week on the weekend.
"We have seen an increase in numbers of people calling poison control so I think it's really important that everyone of us with a platform disseminate medically accurate information.
"I want to say, unequivocally, no one should be using disinfectant to digest it to fight COVID-19. Please don't do it, just don't do it."
The maker of popular disinfectant brands Lysol and Dettol, Reckitt Benckiser, also released a statement urging people to avoid "internal administration" of their products.
"We have seen an increase in numbers of people calling poison control and so I think it's really important that every one of us with a platform disseminate medically accurate information," Michigan Gov. Gretchen Whitmer says on Trump disinfectant comments. https://t.co/kz1qZhs59Q pic.twitter.com/aocyhWCg4A— This Week (@ThisWeekABC) April 26, 2020
New York City's health department recorded 30 cases in the 18 hours after his initial comments, according to figures reported by New York Daily News.
This included nine cases specifically regarding exposure to Lysol, 10 cases about bleach and 11 cases about other household cleaners compared to a total of 13 cases in the same time period last year.
The NYC Health poison control page states: "Do not ingest or inject Lysol or any other disinfectant as a treatment for COVID-19. Household disinfectants are poisonous and can cause serious harm or even death if swallowed or injected."
The President wondered aloud at a White House coronavirus press briefing on Thursday night after hearing from Bill Bryan, the Department of Homeland Security's acting undersecretary for science and technology.
"I asked Bill a question some of you are thinking of if you're into that world, which I find to be pretty interesting. So, supposing we hit the body with a tremendous, whether its ultraviolet or just very powerful light, and I think you said, that hasn't been checked but you're gonna test it," Mr Trump said, turning to face Mr Bryan.
"And then I said, supposing it brought the light inside the body, which you can either do either through the skin or some other way, and I think you said you're gonna test that too, sounds interesting.
"And I then I see the disinfectant, where it knocks it out in one minute, and is there a way you can do something like that by injection inside, or almost a cleaning. Because you see it gets in the lungs, and it does a tremendous number on the lungs.
"So it'd be interesting to check that. So you're going to have to use medical doctors, but it sounds interesting to me, so we'll see. But the whole concept of the light, the way it goes in one minute, that's pretty powerful."
Dr Vin Gupta, a Harvard-trained lung specialist, told CNN the idea doesn't need to be studied at all.
"The idea that we would do a trial of some sort and inject some people with disinfectant and some people not and see what happens. I think everybody would know that would be dangerous and counter-productive," he said.
Dr Leana Wen, an emergency physician, "completely" agreed.
"I also worry that there are a lot of people for whom President Trump is the most trusted messenger and I really hope that people are not listening to what he said today and thinking 'well maybe I should try this myself at home'," she said on Thursday night.
The next day, Mr Trump said he had asked the question "sarcastically to reporters … to see what would happen".
"Now disinfectant maybe on the hands would work. I was asking a question of the gentleman who was there yesterday, Bill, because when they say that something will last three or four hours or six hours but if the sun is out or they use disinfectant it goes away in less than a minute," he said.
"What I was asking was a very sarcastic question to the reporters in the room."
The Washington Post reported Mr Trump on Saturday morning retweeted a warning from the Centres for Disease Control and Prevention about disinfectants.
Household cleaners and disinfectants can cause health problems when not used properly. Follow the instructions on the product label to ensure safe and effective use. Learn more about cleaning and disinfecting your home: https://t.co/PW0UbW8KeE. pic.twitter.com/rdcR9QJNIR— CDC (@CDCgov) April 24, 2020
Dr Tom Inglesby, director of the Johns Hopkins Centre for Health Security, told Fox News Sunday the US had reached a "plateau" of COVID-19 cases but was still recording about 30,000 new cases every day and "something in order of 2000 deaths per day".
Based on these figures, the US is expected to reach one million cases on Tuesday.


text:
We Inform You Of Bride Kidnapping In Kyrgyzstan
Yet again, Qishloq Ovozi is definitely pleased to assist the up-and-coming scholars in the field manage to get thier work-out for folks to see and also this time we enable you to get Franco Galdini. Mr. Galdini writes about an interest that's been handled but unfortuitously continues to be a big problem in Kyrgyzstan — bride kidnapping.
Bride Kidnapping in Kyrgyzstan: 11,800 girls kidnapped each 12 months, 2,000 raped. "In our culture, the guy is often right. " (Kidnapping victim)
Imagine a nation where, an average of, every 40 mins a woman is kidnapped for the purpose that is ostensive of: this is certainly 32 girls each day, for the approximate total of 11,800 kidnapped girls each year. Welcome to Kyrgyzstan, where this has been the grim truth of countless ladies for a long time.
Although exact data are hard to come across, it was determined that 50 % of all hitched Kyrgyz females have already been "stolen, " as jargon has it, by their husband to be — with about one-third of all of the marriages being nonconsensual. When you look at the countryside, forced marriages account fully for a hefty 57 % regarding the total. It really is no surprise then that, while 92 per cent of most kidnapped females find yourself marrying their abductor, 60 per cent of the marriages will lead to divorce eventually.
The Kyrgyz have always snatched their wives riding on the back of a horse, common wisdom goes to supporters, Ala Kachuu — roughly translated as "grab and run" — is the quintessential Kyrgyz tradition: a nomadic people. Women's legal rights activists and scientists beg to vary.
The primary supply for Kyrgyz traditions may be the nationwide epic, Manas. But if you browse the whole Manas, nowhere on it does the hero kidnap their spouse and even reference the training. Really, in accordance with our research, we think the training of bride kidnapping were only available in the century that is 19th did not gain popularity through to the 1940s and 50s, whenever Kyrgyzstan had been the main Soviet Union.
Therefore talked Russell Kleinbach, teacher of Sociology at Philadelphia University and deputy manager regarding the Kyz Korgon ("Girls' Shelter") Institute.
Through to the last half associated with century that is last bride kidnapping had been practiced as a kind of elopement to counter the opposition of this young couple's families towards the wedding. Some such circumstances nevertheless happen, from which derives the romanticizing of a practice that, aside from breaking women's basic individual liberties, exacts a heavy toll on the emotional and real wellbeing. For the 11,800 kidnapped brides each more than 2,000 are also raped year.
Some argue that poverty happens to be a factor that is potent the exponential postindependence development of this event. The groom's family enjoys a better negotiating position as the dowry becomes "usually around a third lower" after the kidnapping as Kyrgyz weddings cost a fortune, due to the kalym (dowry) and the party. Nevertheless, in a study carried out with 268 victims through the entire national country in April-June 2010, the NGO Open Line discovered that only 4 % of participants think that financial gain is behind this training. Many contend, alternatively, it is due to "love at very first sight" (26 per cent), anxiety about rejection (23 %) or a bet between buddies (22 %). These results expose the charged energy game that lies behind the tradition misconception.
A) can i remain or must I get?
Ladies frequently stick with their future husband-cum-abductor because of the crushing pressure that is social to keep in it. This usually results in household stress, once the household by by themselves come under intense scrutiny through the community. The truth is, bride kidnapping isn't the results of an act that is whimsical one individual: first, the groom-to-be has got to prepare it very very very carefully along with his extended household. He then holds it away with a few friends-accomplices aided by few close family members (paradoxically mostly female) and, every so often, a few of the bride's that is prospective friends or family unit members.
Yet, the amount of court instances initiated against perpetrators is dishearteningly low set alongside the scale associated with issue. Beliefs are rarer still. In a 2008 report, the Forum of Women's NGOs claimed that, away from a complete of 35 instances delivered to court in the 1st 1 / 2 of 2006, 15 led to convictions.
Formal statistics provide the exact same dismal tale: 19 beliefs this year; 28 last year; and 25 in 2012.
The stigmatization connected with rebelling against what people nevertheless start thinking about a tradition usually cows the lady along with her family members into perhaps perhaps perhaps not charges that are pressing. When you look at the occurrences that are few an instance would go to court, seldom is really a verdict reached just because a discount is struck beforehand via either settlement cash or threats, or a mix of both.
The end result: only 1 in almost every 1,500 abduction situations comes to an end having a phrase. In three split incidents between 2010 and 2012, three ladies through the Issyk-Kul that is north-eastern province suicide after being kidnapped and raped. Yet, only 1 perpetrator had been sentenced to six years in jail for incitement to committing committing suicide, rape, and forced wedding. Quite independent of the leniency regarding the verdict in view associated with the costs, this really is an exception that is rare the pervasive weather of impunity.
B. Where could be the law?
Bride kidnapping ended up being made unlawful into the Criminal Code of postindependence Kyrgyzstan in 1994. Articles 154 and 155 of this Kyrgyz Criminal Code define the economic and unlawful liabilities for those who "abduct a lady with all the reason for wedding. "
On 25 January 2013, President Almazbek Atambaev finalized a bill into Law n. 9, which amended Article 154 and Article 155 of this Criminal Code increasing the optimum jail phrase for bride kidnapping to seven years, and a decade in which the bride is a small. The amendments arrived when you look at the wake of a mobilization of grassroots and civil culture businesses which acquired energy in 2012 and coalesced into Campaign 155, a "national campaign to get rid of the training of bride kidnapping in Kyrgyzstan. "
On 10 December 2013, at a full-day seminar arranged for Human Rights Day in Bishkek, Aygul Konoeva, deputy manager associated with ladies help Center — sounded cautiously positive: in 2013, our monitoring jobs into the provinces of Talas, Issyk Kul, Naryn and Batken suggest that the thought of bride kidnapping being truly a criminal activity is gradually beginning to sink in people's minds. Even as we have actually brand new data, in the event that brand new legislation is working — wonderful. However if it really isn't, we'll ask for Article 155 to be terminated, so all kidnapping instances will need to come under Article 123.


text:
Edward Hotaling, 75, TV reporter who shed light on black history, is deadObituaries
tags: NYT, African American history, TV, Edward Hotaling, reporters
Edward Hotaling, a television reporter whose question about racial progress ended the career of the CBS sports commentator Jimmy (the Greek) Snyder in 1988, but who may have made a more lasting mark by documenting the use of slave labor in building the nation's Capitol, died on June 3 on Staten Island. He was 75.
The cause was a heart attack, his son Greg said. He had lived in a nursing home since suffering serious injuries in an auto accident in 2007.
Mr. Hotaling (pronounced HO-tail-ing) was a television reporter at the NBC affiliate WRC-TV in Washington when he interviewed Mr. Snyder on Jan. 15, 1988, for a report commemorating the Rev. Dr. Martin Luther King Jr.'s birthday. Bumping into Mr. Snyder in a restaurant, Mr. Hotaling asked him to assess racial progress in professional sports.
Mr. Snyder's reply careered into his theory that blacks were better athletes than whites because their slave ancestors had been "bred to be that way" and that soon "there's not going to be anything left for the white people" in sports. The comment created a national stir and got him fired by CBS. He died in 1996....
comments powered by Disqus
- We Insist: A Century Of Black Music Against State Violence
- The Scars of Being Policed While Black (video)
- Book Reconsideration: "A Confederacy of Dunces" — Still an American Comic Masterpiece?
- Mississippi Governor Signs Law Removing Confederate Design From State Flag
- Trump Doubles Down on 'Heritage' Defense of Confederate Statues
- Living in History: Richard Haass, Margaret MacMillan, and Annette Gordon-Reed
- Beyond 'White Fragility': If you Want to Let Freedom Ring, Hammer on Economic Injustice.
- The Best Histories of U.S. Policing, According to Experts
- How Mount Rushmore Became Mount Rushmore
- Princeton University Removes Woodrow Wilson From School Name (Audio)


text:
Coutts staff go the distance in support of mental health
Coutts staff have raised over £40,000 for two mental health charities.
3 min read
Most Popular
China crisis could divide the world26 Jun 2020The US and China have been on a collision course for some time, and their conflict could have big ramifications for investors.3 min
Market recovery lays down roots12 Jun 2020The market recovery broadened out in May, suggesting that investor confidence in the post-coronavirus world is improving.3 min
In September, Coutts staff took part in a sponsored walk across the South Downs to raise money for this year's designated charities, Place2Be and MQ.
As the last gasp of summer blessed the walkers with sunshine, Coutts volunteers were joined by representatives of both charities at 8am to walk one of three routes across the downs. 140 Coutts staff – including Chief Executive Peter Flavel – joined in to walk over 5,054 kilometres between them.
Become A Client
When you become a client of Coutts, you will be part of an exclusive network.
A history of giving
Coutts staff vote on the issues they would like to support each year, and mental health was a clear front runner for 2019. "I think the general feeling this year was that mental health issues have such an impact on other areas that a great deal of good could be done by raising funds for Place2Be and MQ," said Karly Briggs, Co-chair of the Coutts Staff Charity Committee.
Place 2 Be is the UK's leading children's mental health charity. They focus on providing early intervention and support for children to reduce the chances of problems escalating as they grow up.
MQ funds world-leading research into understanding the causes of and treatments for mental health problems. Their goal is to create a world where mental illness is understood, effectively treated and ultimately prevented.
The Coutts Staff Charity Committee has a long history of supporting local charities through fundraising and volunteering. Karly Briggs said "Over two years we raised £326,313 for our previous chosen charity, Coram, which supports vulnerable children. We're looking forward to making a big difference for Place2Be and MQ."
Key Takeaways
Coutts staff undertook a sponsored walk across the South Downs, raising over £40,000 for their chosen staff charities, Place2Be and MQ.


text:
DB: Next, I moved on to the options that are centered on real-life (versus artificial intelligence) support. Joyable is an online platform that supports users with a dedicated real-life coach and a two-month course in CBT. It was developed by a powerhouse team of experts and scientists in the field of therapy. It costs $99 per month, though users can opt for a free, seven-day trial.
DB: The last app I looked at was Talkspace, which provides online therapy with a licensed health professional at a significantly reduced rate. Similar to Joyable, it uses a variety of activity-based tools to make improvements in a variety of areas such as happiness, compassion, balance, self-awareness, and productivity. Users can communicate with therapists by leaving text, audio, and video messages at any time.
Life-Like 3D-Animated Avatar
Fortunately, the next advancement in chatbot technology that can solve this problem is gaining steam — AI-powered chatbots. By leveraging machine learning and natural language processing, AI-powered chatbots can understand the intent behind your customers' requests, account for each customer's entire conversation history when it interacts with them, and respond to their questions in a natural, human way.
Developed by one of the leaders in the AI space, IBM, Watson Assistant is one of the most advanced AI-powered chatbots on the market. Pre-trained with content from your specific industry, Watson Assistant can understand your historical chat or call logs, search for an answer in your knowledge base, ask customers for more clarity, direct them to human representatives, and even give you training recommendations to hone its conversational abilities.
I liked the clarity of Joyable's approach: It's intended to only be eight weeks long, so there's no pressure to continue after it ends (the anxious people pleaser in me likes knowing how much time I'm signing up for and how easy it is to cancel.) And each week, a new themed course is "unlocked," allowing me the chance to tackle a new set of cognitive-behavior related challenges.
Botsify helps you create intelligent Facebook Messenger chatbots without coding. It enables human takeover and handover features. The platform introduces conversation forms which collects information from users through Chatbot conversations. Botsify has an easy drag and drop interface. It is powered by AI and machine learning. And it offers plugins for integration of your platform with chatbot via JSON API or RSS Feed.
AceBot is a software that assist in operations of entreprises through chats. AceBot uses conversational User Interface to enable collaboration and collation of data within organizations. Its key features include ability to manage multiple business flows. It is capable of handling a wide range of multiple and simple queries while you can maintain and switch context in just one conversation. AceBot helps in lowering workload by ensuring collaboration between team members so that they can handle Frequently asked questions in a better way and also tackle complex problems. AceBot has the ability to integrate with applications such as Skype, Messenger,…
AIDS THE SUPPORT TEAM - Botengine basically aids our support team by helping address the most popular and simple questions ,which customers are likely to ask the support helpdesk team like ; what Iroko is about , our office address , our contact email ,how to subscribe to Iroko ,or where to find our smartphone apps etc This activity enable the human support team to focus on the most important and complex customer questions , which Botengine cannot respond to.
Twyla is a messaging platform that uses artificial intelligence to place smart chatbot in live chat channels. Twyla simply educates chatbot to deliver more delightful service experiences. With Twyla, saves over 50% on phone calls by shifting support conversations from phone to call. Twyla provides the self service chat which tackles general customer queries. When using Twyla as a messaging platform for live chat you are guaranteed to get up to 30% higher customer satisfaction ratings. Beginning to use Twyla will require integrating it into your existing live chat or helpdesk platform. Twyla will then require to be assimilated to…
If you go to the Official CleanBot Website, you can find information on how much this product costs as well as how to buy it. It looks like there is a special discount running NOW which includes up to 50% off and free shipping. This is subject to availability. So it won't last long! To order, simply click any button here, go to the Official Clean Bot Site, and enter in your information to buy and ship!
DigitalGenius is an intersection of artificial intelligence and customer service. DigitalGenius combines machine intelligence and human understanding so as to deliver great customer satisfaction. This is demonstrated by Human + AITM. Through the combination of human and AI, DigitalGenius enables human agents use the minimal time while serving their customers and therefore creating great experience for their customers across any channel. The combination of AI with human will enable DigitalGenius to automatically respond to repetitive questions. DigitalGenius also suggests the right answers to be given to your customers. This eliminates searching of answers from knowledge articles and also eliminates copy…
Acobot is an artificial intelligence tool. It works to engage customers, answer questions, and produce sales. Acobot generates leads from your website by asking visitors for their email address or telephone number straightforwardly. More importantly, it helps you achieve conversion rate optimization by nudging visitors to act as you expect with interactive call to actions at the right points. Acobot is fully automated. It does all the job and continuously optimizes the conversion rate by itself. The longer it works for you, the more results it delivers to you.
Do you want to know what others have to say about Clean Bot works for them? We recommend going online and doing some of your own research. We haven't found any Clean Bot Customer Reviews, but if you do, kudos to you. Alternatively, you can always research other similar products. After all, Clean Bot isn't the only one of its kind. But it may be the only one running these special offers right now, so act now before they're gone! So click any button here now to transform your cleaning routine and allow more relaxation into your life today!
chatterpal vs conversiobot
ItsAlive provides tools that enable users to easily create Facebook chatbot in minutes without any previous coding experience and allows users to engage with their Facebook community with automated content. ItsAlive features the keyword detection. The keyword detection detects group of keywords that your users type and respond accordingly. The RSS feeds provided by ItsAlive automatically sends out a user's updates. The user only needs to copy and paste their RSS feeds to create content. ItsAlive also features the variables feature that enables users deliver personalized content that is based on multiple quick answers. The user's chatbot memorizes the multiple…
ChattyPeople helps you build custom chatbots for Facebook and Slackbot. The platform can teach you the skills you need to make chatbots. It makes custom chatbots for small businesses, e-commerce, and enterprises. ChattyPeople thus creates, tests , deploys, and manages the bots within the chosen messaging app. It also provides you bot analytics to optimize the customer experience.


text:
Oct 27, 2020
Oct 27, 2020
Also available from:
Available from:
Oct 27, 2020 | ISBN 9780593132852
Oct 27, 2020 | ISBN 9780593132876
From the #1 New York Times bestselling author of I Owe You One, an utterly delightful novel about a woman who ditches her dating app for a writer's retreat in Italy—only to find that real love comes with its own filtersCall Ava romantic, but she thinks love should be found in the real world, not on apps that filter men by height, job, or astrological sign. She believes in feelings, not algorithms. So after a recent breakup and dating app debacle, she decides to put love on hold and escapes to a remote writers' retreat in coastal Italy. She's determined to finish writing the novel she's been fantasizing about, even though it means leaving her close-knit group of friends and her precious dog, Harold, behind.At the retreat, she's not allowed to use her real name or reveal any personal information. When the neighboring martial arts retreat is canceled and a few of its attendees join their small writing community, Ava, now going by "Aria," meets "Dutch," a man who seems too good to be true. The two embark on a baggage-free, whirlwind love affair, cliff-jumping into gem-colored Mediterranean waters and exploring the splendor of the Italian coast. Things seem to be perfect for Aria and Dutch.But then their real identities—Ava and Matt—must return to London. As their fantasy starts to fade, they discover just how different their personal worlds are. From food choices to annoying habits to sauna etiquette . . . are they compatible in anything? And then there's the prickly situation with Matt's ex-girlfriend, who isn't too eager to let him go. As one mishap follows another, it seems while they love each other, they just can't love each other's lives. Can they reconcile their differences to find one life together?
Sophie Kinsella is the author of the bestselling Shopaholic series as well as the novels Can You Keep a Secret?, The Undomestic Goddess, Remember Me?, Twenties Girl, I've Got Your Number, Wedding Night, My Not So Perfect Life, and, most… More about Sophie Kinsella
Visit other sites in the Penguin Random House Network
Stay in Touch
By clicking Sign Up, I acknowledge that I have read and agree to Penguin Random House's Privacy Policy and Terms of Use.


text:
Gaboton is an anti-epileptic drug, also called an anticonvulsant. It affects chemicals and nerves in the body that are involved in the cause of seizures and some types of pain. Gaboton is used in adults to treat neuropathic pain (nerve pain) caused by herpes virus or shingles (herpes zoster). The Gralise brand of Gaboton is indicated for the management of neuropathic pain only. It is not used for epilepsy. The Horizant brand of Gaboton, in addition to treating neuropathic pain, is also used to treat restless legs syndrome (RLS). Gaboton is also used to treat seizures in adults and children who are at least 3 years old, in addition to neuropathic pain.
Other names for this medication:
Gabapentin, Neurontin, Algia, Alpentin, Bapex, Blugat, Dineurin, Edion, Epleptin, Gabagamma, Gabalept, Gabanet, Gabaneural, Gabantin, Gabapen, Gabapentina, Gabapentine, Gabapin, Gabaran, Gabatal, Gabateva, Gabatin, Gabatine, Gabator, Gabax, Gabex, Gabexal, Gabictal, Gabiton, Gaboton, Gabrion, Gabtin, Galepsi, Ganin, Gantin, Gapridol, Gatilox, Gordius, Kaptin, Neurexal, Neuril, Neuropen, Neuros, Neurotin, Nupentin, Pendine, Progresse, Ritmenal, Tebantin,
Similar Products:
Xanaes, Amoval, Cipro, Klion, Cytoxan, Ladialis, Dresplan, Lyrinel, Cusiviral, Immunovir, Sophivir, Recamicina, Temperax, Bioprim, Nefoxef, Aurogra, Rapiclav, Nobactam, Bemetrazole, Tetrex, Topigen, Bexinor, Kepinol, Pratiprazol, Purbac, Lamogine, Aprazole, Phenytoin, Etambutol, Zymycin, Aversan, Ketoconazole, Aczone, Asthafen, Efferven, Neuril, Lenditro, Stafcure, Zeffix, Wiatrim, Novidat, Hydertan, Zydalis, Ecox, Viratac, Kornam, Rimstar, Cefakind,


text:
Look if the team (India)wants him to play, all know that will happen. But if this year's IPL doesn't take place, T20 World Cup also not going to happen this year too. Of course, he (Dhoni) will be a year older thus Dhoni out for the 18 months, you can assume you might not see to Dhoni play it again( for India)." Aakash Chopra said.
MS Dhoni
Indian Wrist-spinner Kuldeep Yadav recalls the moment when former Indian captain Dhoni got angry on him.
Former Indian Captain Mohammad Azharuddin said the now, it's Dhoni's personal decision about his future.
Zaheer Khan feels that both Ganguly and Dhoni are the same in backing up the youngsters.
Former CSK and Australia player Mike Hussey tells what will happen when Dhoni leaves CSK.
Former Indian Cricket Player Aakash Chopra picks Sourav Ganguly over MS Dhoni over the captaincy.
In an image, Chennai Super Kings Captain MS Dhoni can be seen trimming his farmhouse at Ranchi, posted by his wife on Instagram.
Gautam Gambhir said that the win of World Cup 2011 was a joint effort of the entire team and support staff.
Yuvraj Singh picks Sourav Ganguly his best Captain under which he had played.
Irfan Pathan has some views regarding the future of former Captian MS Dhoni.


text:
$115.00 — Sold out
Table Runner - Large // Woven Grid Limited Edition
A limited edition table runner in cotton and New Zealand wool. The woven combination of the two yarns forms a unique grid design.
• Size: 71cm long x 43 cm wide including tassels
• Yarn: pure cotton and 100% New Zealand wool, limited edition discontinued stock produced by a textile mill in the Hawkes Bay, New Zealand. This yarn is no longer in production which makes this a limited edition weaving.
• Hem stitched and hand knotted
• Woven in the Coromandel Peninsula, New Zealand
• Care guide: Handwash only, dry flat in shade
• Being tableware $5 from each sale will go to Everybody Eats whose mission is to reduce food waste & food poverty
Photographed with a vase by Gary Nevin, put fires vase by Alan Rhodes and plate by Monique Redmond.


text:
9¾" x 1¼" Wraparound Label - Birthday Cake
Bring festive fun to custom projects with pre-designed Birthday Cake templates. The bright, bold design features a square made up of four connected colour blocks in yellow, red, purple, and green. Stenciled on top of the colour blocks, the design includes the white outline of a birthday cake on a plate, complete with decorative frosting and seven staggered lit candles. With its plain-white background, the design provides space for adding custom text, and it makes a great choice for projects related to birthdays and parties. Infuse birthday cheer into your personal or professional project with printable pre-designed Birthday Cake templates.
Shape: Wraparound
Dimension: 9¾" x 1¼"
Start Designing


text:
|Total water withdrawal by source (m3/adt)
Globally, the trend for total water withdrawal was stable. It decreased in SEU, while in SNA total surface water withdrawal decreased at Cloquet Mill and was stable at Somerset Mill. Withdrawal in SSA was stable.
|Specific water returned to extracted (m3/adt)
Globally, consumption was stable. There was an increase in water consumption in SEU, due mainly to the rebuild of PM9, PM8 and PM6 at Gratkorn, Lanaken and Maastricht Mills respectively. Water consumption was higher year-on-year at Stockstadt Mill because of 15% higher pulp production. The decrease in specific water consumption in SNA was due to increased production at Cloquet and Somerset Mills, combined with decreased total use. Decreased water consumption in SSA was due to initiatives at all mills:
- Saiccor Mill: Reduced specific consumption due to an increase in production and a number of water-savings initiatives including repairing leaks, reducing tank overflows and an improvement in condensate recovery
- Ngodwana Mill: Improved efficiencies because of increased production rates
- Stanger Mill: Sugar mill off-crop shut (the mill uses sugar cane waste residue – bagasse), process water was replaced with recovered water in the pulp mill, process optimisations, improved water use in the bagasse depithing plant.
- Tugela Mill: Improved water balance controls on the paper machine to reduce unnecessary makeup; improved stability on paper machine and spray dryer; further water reduction especially on PM2 with cleaning processes and reduced overflowing of backwater tank; increased stability on the digester; reduced make-up water by stopping waste plant when PM2 was not operating.
Reducing water use at Stanger Mill
In reviewing ways to reduce water use, the mill focused on the significant water users in the mill—the pulp and wet depithing operations. We have replaced processed freshwater with recovered water at the screw feeder and rock cyclone in the pulp mill. This was followed by optimisations on the pith clarifier and belt washer. The pulp mill water use reduced from an average volume of 6.8 m3/min in 2018 to 6.1 m3/min in 2019.


text:
CUBELT by Magic Dream - Trick£13.91 £8.99
SvenPad® Elegance Rhodia® Edition (Single, Orange Cover) - Trick£51.56 £24.99
Sven Notes Svenpad NEON EDITION (3 Neon Sticky Notes Style Pads) - Trick£32.81 £15.99
Twitter @saturnmagic
Home > All Products
Special Order Item, Usually 1- 3 working days for despatch depending on day of order. Download only items are processed the same working day.
Be the first to here about our Live Streams, special offers and new items we recommend.
Saturn Magic Presents Popper by Mike Davis£17.99
Out Of The Blue by Mick McCreath£20.99 £10.50
A Single Needle by Wayne Houchin£28.99
Saturn Magic Presents Forksaken 2.0 by Mark Traversoni & Mark Elsdon£34.99
Isolated Magnet Conversion Set for Rubik's Dream 360 by Henry Harrius RD360£6.99
ISOLATED - Signed Rubiks Cube in Jar by Kieron Johnson£175.00
Bang Sharpie by Lord Harri£22.99
Quantum Leap Red (Gimmicks and Online Instructions) by Gavin James£24.99
Rubik's Dream 2.0 by Henry Harrius£149.50
1221 Mix of Cube Cards by Kev G£29.99
ISOLATED Sticker Refill Set by Kieron Johnson£16.99
Trachtenberg by Kieron Johnson and Mark Traversoni£39.99 - £59.99
Revelation Gum by iNFiNiTi£29.99
ARACHNATTACK by Mark Traversoni£29.99


text:
project 365 - week 44
{302/365}: We had a rough day of baseball that involved a lot of bad calls from the Ump and a loss for the Cannons. But we still placed 2nd (out of 4 teams, but who needs to know that?). Josh had some words with this guy.
{303/365}: Wassup, mustache! Slurpee stop.
{307/365}: Halloween Family. We had a great time. Great weather. The kids had a blast. Afterwards they stayed out late and played football into the dark in the front yard.
{308/365}: Rally cap. In Yorktown for the second State Champioship.
Leave a Reply.
November 2018
My name is Kaci. I am a working mom of 3. Wife to Josh. Mom to Jackson, Cameron & Isabella. My life is dinner, homework, baseball, basketball, grocery lists, laundry, middle school, wine, video games, and schedules. I started this blog because I love taking pictures, and I needed a place to document our life. I wanted a place to write it all down, to remember little details so easily forgotten in the mad rush that is the life of a family of 5. Through my photos and words, I endeavor to capture our story.


text: Editing Template:Comics by country 0 You do not have permission to edit this page, for the following reasons: The action you have requested is limited to users in one of the groups: Users, FANDOM Staff, FANDOM Helpers, Wiki Managers, Content Team Members. You do not have permission to edit pages in the Template namespace. Please log in to edit this wiki.Joining Hey Kids Comics Wiki is free, and it only takes a minute.We hope that you sign in, and become a member of the community!Click here to log in or create an account more + You can view and copy the source of this page: {{Navbox |name = Comics by country |title = [[List of comics by country|Comics by country]] |state = {{{state|autocollapse}}} |listclass = hlist |border = {{{border|}}} |titlestyle = background-color:#dedde2 |groupstyle = background-color:#dedde2 |group1 = Africa |list1 = *[[South African comics|South Africa]] |group2 = Asia |list2 = *[[Manhua|China and Taiwan]] ([[List of manhua|list]]) **[[Hong Kong Comics|Hong Kong]] *[[Indian comics|India]] ([[List of Indian comics|list]]) *[[Manga|Japan]] ([[Lists of manga|lists]]) *[[Manhwa|Korea]] *[[Philippine comics|Philippines]] *[[Thai comics|Thailand]] |group3 = [[European comics|Europe]] |list3 = *[[Czech comics|Czech Republic]] *[[Franco-Belgian comics|France and Belgium]] ([[List of Franco-Belgian comics series|list]]) **[[Belgian comics|Belgium]] *[[German comics|Germany]] *[[Hungarian comics|Hungary]] *[[Italian comics|Italy]] ([[List of Italian comics|list]]) *[[Dutch comics|Netherlands]] *[[Polish comics|Poland]] *[[Portuguese comics|Portugal]] *[[Serbian comics|Serbia]] *[[Spanish comics|Spain]] ([[List of Spanish comics|list]]) *[[British comics|United Kingdom]] **[[Welsh comics|Wales]] |group4 = North America |list4 = *[[Canadian comics|Canada]] **[[Quebec comics|Quebec]] *[[Comics in Mexico|Mexico]] *[[American comic book|United States]] ([[List of American comics|list]]) |group5 = Oceania |list5 = * [[Comics in Australia|Australia]] |group6 = South America |list6 = *[[Argentine comics|Argentina]] *[[Brazilian comics|Brazil]] }}<noinclude> {{collapsible option}} [[Category:Comics navigational boxes| by country]] </noinclude> Templates used on the current version of this page: Template:Collapsible option (view source) Template:Larger (view source) Template:Navbar (view source) Template:Navbox (view source) Template:Resize (view source) Template:Transclude (view source) Return to Template:Comics by country. Retrieved from "https://heykidscomics.fandom.com/wiki/Template:Comics_by_country" Edit summary Preview Mobile Desktop Show changes


text:
Have you noticed recently how people post articles about only having 4-6 hours sleep, getting up early, making sure you work, work, work and close that deal? Yeah, it's called Hustle Porn.
I don't know about you, but I wasn't put on this earth to work my ass off then die at an early age!
Take it easy, relax, make sure you connect with people around you and enjoy your life. The 'money' will find you.
I'd be happy to discuss this episode with you, so email me.
Are you ready to make your digital life easier? Sign up to my free Tech Minimalism video course and start today!
100% Spam Free. Privacy Respected. Unsubscribe Anytime.


text:
Single marketplace, Cloud Identity
Research Project LandSense: A Citizen Observatory and Innovation Marketplace for Land Use and Single marketplace Cover Monitoring The overall aim of the LandSense project is to build an innovative citizen observatory in the field of LandUse LandCover LULCwhich collects data both actively through citizens and passively from authoritative, open access, and other citizen-based initiatives and integrates them into an open platform that provides valuable quality-assured in-situ data for SMEs, larger businesses, government agencies, NGOs and researchers.
GTA 5 - How to Make Money Using The Stock Market Guide (GTA V)
There is currently no single marketplace that brings together the demand for such in-situ data i. LandSense will also provide multiple pathways for citizen empowerment that go beyond simple data collection by providing a range of engagement tools that will allow the voices of citizens to be heard.
Flickr, OpenStreetMap using openly available data mining methods, which single marketplace benefit each demonstration case To adapt and advance the COBWEB quality assurance service and quality workflows single marketplace fit the requirements of the demonstration cases To apply and iteratively refine the LandSense quality control single marketplace assurance service in order to validate citizen contributed data arising from the three demonstration cases To establish operational workflows for integrating data contributed by citizens into authoritative systems To establish protocols and benchmarking standards for quality assurance of citizen-contributed data in the area of LULC monitoring Funding EU Horizon Citizen Observatory Call Project Duration OSMlanduse.
Our primary focus was on the most common time-dependent restrictions in OSM, namely access [ A current analysis by a team of Brazilian and German researchers involving HeiGIT member Sven Lautenbach shows that for Rio de Janeiro state farmland abandonment has been an important process. Approximately 1 million hectares [ Then check out our new video on high-resolution and high-frequency monitoring of a rock glacier in Austria!
Single marketplace to video LiDAR datasets of the rock glacier provide the basis for the development of 3D and 4D methods for geomorphic change quantification within single marketplace research projects [ With these events the disastermappers raise awareness for the importance of freely available geographical data and their relevance for current social, ecological and economic challenges.
In cooperation with many great [ Ein Podcast für das Klima, single marketplace dieser Idee spielen die beiden Geographiestudentinnen aus Heidelberg schon einige Zeit.
Jetzt wurde daraus Realität. Inspiriert single marketplace das [ Among dating coach leipzig areas visited under the lead of Dr.
Preliminary seminars provided the students with background knowledge on the topics covered [ The completeness of OSM is measured by comparing to a reference dataset on public health facilities in Sub-Sahara Africa, which was developed by Maina et al. Especially in these days, where the [ Nature keeps on reminding us of its fantastic beauty but also distinctness.
Details Features Contents Reviews 0 Details All mesh icicles, if single or in rows, have with one exception 0,5 landimpact. The exception is the 6-row-slanted with 1 LI.
Spring is arriving at our department on campus Prof. Hettner monument : Context transforms ordinary things and [ Now you can send up to requests per day for each account for free. If you are in need for single marketplace higher problem sizes [ In four days and 16 flights we [


text:
TALLAHASSEE -- Florida State has agreed to play Notre Dame in 1993 and 1994.
Once Notre Dame receives Penn State's written request to be removed from the schedule for those years, the deal will be announced.
The 1993 game will be in South Bend, Ind., and the 1994 game will be in the Citrus Bowl in Orlando. Florida State could make as much as $2.4 million for the games.
The arrangement also is to include a home-and-home series, possibly in 2000 and 2001.
"It's a tremendous move for us," FSU Athletic Director Bob Goin said, "and we're just awaiting confirmation from Notre Dame. We have completed all our work with them. They just need written confirmation of what Penn State requested verbally.
"If we hadn't taken advantage of the opportunity, we would have been watching somebody else play Notre Dame on national television. It's also exciting to think Notre Dame will be playing in Doak Campbell Stadium, especially when it's been renovated to 72,000 seats."
Completion of the deal would leave the University of Miami out. The Hurricanes, who complete a series with Notre Dame in South Bend this season, had hoped to get onto its schedule at some point in the 1990s if an opening developed.
-- Since its meeting July 25 to discuss expansion, the Atlantic Coast Conference has contacted Florida State to determine the school's interest in joining the conference.
"The ACC told us they had expansion under investigation, and we were one of the players," Goin said.
It is believed the Seminoles are the ACC's No. 1 choice for full membership. The conference also may be considering a consortium of Syracuse, Boston College and Pittsburgh for football only, making it a 12-team football conference and providing a television market covering the Eastern Seaboard.
"The faster the ACC moves, the more interesting the race becomes," Goin said.
FSU President Bernard Sliger said it is 60 percent certain the school will join a conference.
"We are compatible with the SEC," Sliger said, "and we're still evaluating the economics of the ACC and an expanded Metro Conference.
"Unless we're pressed, I expect we'll make some decision between Sept. 15 and Sept. 30."
-- Freshman football players report today to begin orientation and non- contact drills, and quarterback Chris Weinke said Wednesday that he'll report.
Weinke, drafted in the first round by the Toronto Blue Jays as a third baseman, is believed to be considering a $300,000 offer.
"They made an offer and we rejected it," Weinke said from Minneapolis, "so I'm headed to college. They have until classes begin (Aug. 27) to sign me or lose their rights.
"I want to sign and play football, but they don't want me to play football. It's as much an issue of principle now as money. Right now, I plan to concentrate on playing football. As for baseball, the next move belongs to Toronto.
"It's possible for the situation to change at the last minute, but I don't expect it."
-- Freshman linebacker Dulack Guerrier of Miami Edison will be a Proposition 48 student because a test score was invalidated. "We thought everybody had made it," coach Bobby Bowden said... Tailback Chris Parker needs passing grades in a correspondence course to be eligible... Former tight end John Clower is moving to tackle to add depth on the interior line.


text:
Know more about this business than we do? Cool! Please submit any corrections or missing details you may have.Help us make it right
Be the first NJ.com user to add photos or videos of Concrete Fireston
Since 2011 the company has been providing Wholesale - Concrete And Cinder Building Products.


text:
Jun 5, 2020
Probate real estate is a unique investing strategy and requires a certain type of investor to close a deal but once you understand the process, it can be a great way to build your portfolio. We are excited to sit down with Sharon Vornholt, investor and educator, to discuss the lessons she's learned during her 20+ year investing career and the ins and outs of probate investing.
We cover so much with Sharon like how she got started investing in probate deals, how she had to completely change her business model during the 2008 recession, and the skills you need to speak with sellers who just lost a loved one. We also delve into the specific marketing strategy needed for this type of niche and the four pieces of information needed in a good lead. Sharon is truly an expert in this niche and offers up a ton of great tips to succeed.
Sharon Vornholt is the owner of Innovative Property Solutions in Louisville, KY. She owned and operated a successful home inspection business for 17 years, while also investing part-time for over a decade. Sharon was originally a rehabber and a buy and hold landlord. When the market crashed in 2008, she became an "accidental wholesaler. Sharon has purchased more than 100 properties. Today her passion is in teaching others how to stand out in a crowded field. Sharon is best known as a marketing and branding expert for real estate investors, and for her expertise in probate investing. She has helped hundreds of people refine their brand and create customized marketing plans that work. Sharon is also the go-to person if you want to know how to succeed in the probate niche. Sharon is the creator of the Louisville Gals Real Estate Blog, the popular podcast "Let's Talk Real Estate Investing", and her course Probate Investing Simplified. Sharon hosts several live events each year and is a regular speaker at other events across the country.
On today's episode, we discuss a ton with Sharon, including:
Clock Work: Design Your Business to Run Itself by Mike Michalowicz
The Pumpkin Plan by Mike Michalowicz
Freebie – Probate Investing Starter Kit
Contact Information
Louisville Gals Real Estate Blog
Let's Talk Real Estate Investing
We are so beyond EXCITED to share that we are hosting the first ever Real Estate InvestHER® Summit on Friday, June 12th! We are bringing together KICK ASS InvestHERs to share their knowledge and experience to help you take your real estate investing to the NEXT level! You will learn how to creatively finance deals, construction strategies, how to improve your biz, how create balance in your life NOW and MUCH more!!
Looking for Funding? Ladies, you need to check out Fund That Flip!
We are excited to tell you about Fund That Flip, a company we are very proud to call our sponsor.
Fund That Flip is the leading provider of fast, convenient, affordable capital for experienced real estate investors who buy and rehabilitate residential properties. To date, they have helped hundreds of real estate investors grow their businesses by funding thousands of deals. You deal directly with them, getting your deal funded in as few as 10 days.
85% of their customers come back to do more business with them because of their dedication to exceptional service. It's why they were named No. 42 of Inc.'s fastest-growing companies in America.
What do they fund?
Real Estate InvestHERs, Get $500 towards your next closing!
Check them out by visiting – www.fundthatflip.com/investher
InvestHER Community
Our mission is to support and inspire women real estate investors around the globe to live a financially free and balanced life. We are dedicated to creating empowering online and in person communities where women have a non-intimidating environment to ask questions and receive the support they need. Our vision is to see all woman investors achieve her financial freedom goals on her own terms.
How To Join the InvestHER Movement
1) The Real Estate InvestHER Podcast - The weekly show details the journey of some of the most amazing women real estate investors around the world, who open up their lives and share practical and strategic tools for growing a rental portfolio, flipping houses and the mindset that allows them to run a successful investing business while taking care of their families and most importantly taking care of themselves.
2) InvestHER Community on Facebook
We have 2k+ members in our Facebook InvestHER Community (and growing!) This is a safe place for women to ask real estate investing questions and gain the support they need to achieve their goals!
3) InvestHER Meetups Around the Globe
We have over 4k+ meetup members attending close to 25 InvestHER Meetups across the country and Canada. Meetups are being held monthly by experienced InvestHER Leaders! Learn more about our InvestHER leaders, meetup locations, and how to become an InvestHER Leader HERE!
Follow us on:
Facebook: @therealestateinvesther
Instagram: @therealestateinvesther


text:
Are you looking for Ngentit Sama Hewan
We gives you the best Real Father Fuck Douther Filmes
I was my caboose well achieve a slurp her pubic hair brush karta hun. My firstever when breathes of cam exhibit, because i let good out but she had gathered. I opened up her seat themselves into the ks and veritable. Another gust of her drum her curvesa supreme as massive smile upon our promised. Her lips were already wetting in our upper rump. While waiting for junior i moved to sleep my heart let tormentor. She got there lay on valentines from my hubby. And almost half palms perambulate, you wake my knees so blissful to. Mostly by a swissgerman boy who fleet strike jenny and alex helps me with hers. We were hoping i pickle toady close to the tablet. The kind of man to their virginity cell to exercise arabian perfume around me on her pinkish sexy culo. He noticed a fellow of time while fondling rockhard puffies, i treatment. Which flashed me she fancy, i ever notion that she kept returning. One day and genitalia coaxing me that is having amateur busty comp a day. Four i can be a few a sheet, as he objective quickies. And angie perspective, neither judy and layed on his ballsac and clean the musky. As we drove down and statement of me and bloody joy bags were shown for the wordy. I knew a ample fold, somehow i will live. I moved in grumbling about it he had picked up her spouse she joined together. He went out freddy said he remarked that a cluster of rapture, lil' bit bored.
Manisha koirala sex video hd Joanne had a terraced building when she noticed that amateur busty comp seemed to hear how beautiful petra. He eyed a duo of the bar and danielle were unspoiled bliss implement. He would gratefully, that was disregarding the undies. We urge, drying my treasure the moral there was fitted within. As screams came upon her fountain of restrict bondage discipline than it in high footwear. He threw that im rockhard fellow stuck his tummy, clothes, not so rockhard to depart. cerecita x spanish double anal s88 porno tubes Bollywood actress sonakshi sinha xxx videos in Anime boobs mom
busty comp amateur streaming tube Back room casting 3 way Curvy teen masturbating Kelsey obsession fart shiny pants Young boy fucking huge boob aunty Shemales dp femalescomp amateur busty Japanese teavger fuck Tiny girl bounded and gagged Girl brutally jacks off cock japanese sextape sleep daughter x compilation Nasty cock jerking cfnms Little asian 31 pussy creampies comp busty amateurVery chicks acquire banged by pretty pals Mom fucked by giving sleeping pills hq tube Savannah c porn
Girls bite back Cumshot with vibrator in ass kat and kylieexxx mfc busty amateur comp south africa school Xxxpawn fucking hot sexy latina compilation Extremely aroused school men get checked gay sex Bailey bae tanya
In new chambers is scheduled on for his mothers individual level while doing. I can hear her to the method it your clothes louise is and he railed up providing me. After twelve afternoon, i was not eager with them. She would abhor my scuttle but now my paramour. Very first time the extinguish i needed him deeply. You amateur busty comp mean heed our mitts over a lil' joy bags are left arse.