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Technologies in Exploration, Mining, and Processing INTRODUCTION The life cycle of mining begins with exploration, continues through production, and ends with closure and postmining land use.Contact Supplier
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Home / News / Drilling Knowledge / Drilling Techniques for Mineral Exploration Drilling Techniques for Mineral Exploration May 10, 2016 | Drilling Knowledge; In this article Dando looks at the three different types of drilling used for mineral exploration and the pros and cons of each. These drilling techniques are: ... Requiring more equipment ...Contact Supplier
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[Update] Former Naughty Dog employee says he was sexually harassed, fired, and offered $20K to keep quiet
UPDATE: Naughty Dog has made an official comment on Ballard's sexual harassment allegations claiming they have "not found any evidence of having received allegations from Mr. Ballard." The full statement was posted to Naughty Dog's official website, …
Top Playstation studio Naughty Dog responds to allegations of sex harassmentPolygon
Former Naughty Dog Employee Says He Was Sexually Harassed (Update)PlayStation LifeStyle
Top Upcoming PlayStation 4 Exclusives of 2018Gameranx (blog)
Gamechup –GameTransfers
all 15 news articles »
Source: https://news.google.com/news?cf=all&hl=en&pz=1&ned=us&topic=tc&output=rss

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text: Radioactive waste dispute threatens rare earth producer Lynas' future By William Clarke Published: Wednesday, 03 April 2019 The auditors of rare earth producer Lynas have warned that an ongoing legal dispute with the Malaysian government is at risk of threatening the company's future. Auditors Ernst & Young warned in a note on Lynas' quarterly results on February 28 that conditions issued by the Malaysian government "cast significant doubt about the consolidated entity's ability to continue as a going concern." In December 2018, Malaysia's Atomic Energy Licensing Board set new pre-conditions for Lynas' licence... This is a preview of the full article 2 years pricing data on all minerals The latest global news and features Print magazine Article archive ranging from 1988 Access on the move with IM Insight mobile app Take a Trial or Subscription today. Start below: Free Trial OR Subscribe


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Usda Aphis
Marlin Enterprise Providers Corp. Enterprise Services appears for student workers to assist on accounting tasks, submitting and processing of documents, net tech help, and print and copy services. Traditional network administration methods and expertise-centric monitoring approaches are incapable of determining the enterprise impact of a problem in such an advanced infrastructure surroundings.
Incumbents usually supervise seven to 12 workers of which one or more are Enterprise Service Assistant (Specialist) or Business Service Officer I (both Specialist or Supervisor). Or, market your online business to clients for those particular events after they favor to dine in-complete with restaurant-quality meals and repair.
The business services industry is a very broad trade encompassing many alternative classes of enterprise operations; all of them present some type of non-monetary service to other firms. Even the main bookkeeping program for small business, whereas it has a default choice for eating places, fails to provide all of the accounts that most restaurant owners require.
5. Providers franchises are usually very people-oriented, and this holds true for enterprise services franchises as nicely. KPMG introduces six key parts for achievement companies must take into account as they construction their business services in the digital age.
Advocates of BSM often use it to support a change from a tradition which is very technology-focused to a place which understands and focuses on enterprise aims and advantages. Because of the variety of companies and services which can be contained within this business, it is very onerous to make estimations on trends for the business as a whole.
Grab your bucket, squeegee, and glass-cleaning resolution, and rap on the dirty home windows of local businesses and residences alike. Somewhat than supporting an internalized technology view, there is a shift to recognize and support customer needs and the delivery of value to business stakeholders together with shareholders.
Daily, KPMG's World Enterprise Providers (GBS) advisors assist organizations obtain new levels of efficiency, agility, efficiency, value, digital maturity and impression by remodeling enterprise services like procurement, human assets, IT, or finance and accounting.


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NEWS – Yeditepe University students presented the "Portable Heating and Ventilation Project" which costs ₺70 and uses less electricity compared to current products.
Yeditepe University Faculty of Architecture Industrial Design Department and Faculty of Engineering Mechanical Engineering Department students introduced the "Portable Heating and Ventilation Project" at an exhibition organized in the university.
Prof. Dr. Hojin Ahn (Erdem An) from Mechanical Engineering Department and Industrial Design Department lecturer Ergin Yetkin managed the product project which heats in the same way as current products but consumes less electricity.
The product which is made up of two fans costs only ₺70.
Ergin Yetkin emphasized the importance of interdisciplinary work:
This is a study which brought mechanical engineering and industrial design students together for 14 weeks. In business life, these disciplines have to work together. That's why we wanted students to experience this through project lessons. There are several companies that support us. Together with these companies, our products will be put into production and come to a level that can be used in daily life.
Prof. dr. Hojin Ahn expressed his happiness in working with the Faculty of Architecture and continued as follows:
Within the scope of mechanical engineering thermal system design courses, we were generally designing but it was conceptual. But in this period we decided to cooperate with the Department of Industrial Design and this was very different from the experiences.


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Joya de Nicaragua is paying tribute to the visionary businessmen that helped shape the Nicaraguan cigar industry with its latest cigar, Cinco Décadas Fundador.
Cinco Décadas Fundador honors Juan Francisco Bermejo and Simón Camacho with an elegantly crafted cigar. Cinco Décadas was introduced in 2018 as part of Joya de Nicaragua's 50th anniversary. The latest cigar in the Cinco Décadas line pays tribute to key characters that shaped the story of its company. Cinco Décadas Fundador commemorates the vision of tow immigrant businessman that had a great impact on Nicaragua's cigar industry as well as the Joya de Nicaragua brand.
"When we conceived the concept of the brand, we decided that every year until the next big anniversary, we would nationally release a size that would pay tribute to key characters that shaped the story of our company, and thus, today we commemorate the vision of two immigrant businessmen that transformed our country," said Dr. Alejandro Martinez Cuenca, chairman and owner of Joya de Nicaragua.
"This stunning cigar comes in a 6 x 54 soft pressed format that will captivate you the moment you light it," he added. "This Gran Toro comes in a 10-count box with an MSRP of $20 per stick, and will only be available at selected retailers around the world. In the United States it is a DDRP (Drew Diplomat Retailer Program) Exclusive product, that will be shipping as of July 2019."
Cinco Décadas, with a perfect construction is made exclusively with Joya de Nicaragua's prime extra-vintage leaves taken from its most exclusive collection of tobaccos. It carries an immaculate balance accompanied by a luxurious complexity of sweet and spicy flavors. Its silky-smooth smoke delivers a rich and fulfilling experience.
Cinco Décadas Fundador will debut at the 2019 International Premium Cigar & Pipe Retailers Association (IPCPR) trade show and convention in Las Vegas and also at InterTabac in Dortmund, Germany in September.
For all the latest news from Joya de Nicaragua, visit joyacigars.com. Joya de Nicaragua is distributed by Drew Estate in the U.S. For all the latest Drew Estate news, visit drewestate.com.


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EPN Resources
This service provides orbital elements, of Near-Earth objects. The database provides for each asteroid, orbital elements and their uncertainty, the state-vector, information about the observations, MOID, and the covariance matrix of the system, as well as magnitude information. The database is updated daily.
Creators: J. Desmars
Contributors: J. Desmars, W. Thuillot, D. Hestroffer, P. David, P. Le Sidaner, PADC
Publisher: Paris Astronomical Data Centre - IMCCE
The Auroral Planetary Imaging and Spectroscopy (APIS) service provides an open and interactive access to processed auroral observations of the outer planets and their satellites. Such observations are of interest for a wide community at the interface between planetology and magnetospheric and heliospheric physics. APIS consists of (i) a high level database, built from planetary auroral observations acquired by the Hubble Space Telescope (HST) since 1997 with its mostly used Far-UltraViolet spectro-imagers, (ii) a dedicated search interface aimed at browsing efficiently this database through relevant conditional search criteria and (iii) the ability to interactively work with the data online through plotting tools developed by the Virtual Observatory (VO) community, such as Aladin and Specview. This service is VO compliant and can therefore also been queried by external search portals of the VO community. The diversity of available data and the capability to sort them out by relevant physical criteria shall in particular facilitate statistical studies, on long-term scales and/or multi-instrumental multi-spectral combined analysis.
Creators: Laurent Lamy
Contributors: Florence Henry, PADC
Publisher: Paris Astronomical Data Centre - LESIA
The database of planetary images (BDIP) comes from the digitization of photographs collected and preserved by the Center for Photographic Documentation of the planets held by the IAU at the Meudon Observatory in 1961 under the curation of J.H. Focas (IAUC, 12th General Assembly Report, 1964). A similar center was established at the Lowell Observatory in Arizona, under the responsibility of W.A. Baum. The photographs were duplicated between the two centers. Digitization was performed in 1998-2000, funded by the Science Council of the Observatory of Paris.
Creators: Florence Henry
Contributors: PADC
Publisher: Paris Astronomical Data Centre - LESIA
Pic du Midi de Bigorre in the French Pyrenees is the place where coronagraphic images were first realized, by Bernard Lyot in the 1930s. Since then, the solar instruments at Pic du Midi regularly provide images of the solar disc, solar prominences and solar corona.
Creators: Patrick Maeght
Contributors: J.M. Glorian
Publisher: ov-gso
This service publishes spectral matrix data from the Earth magnetosphere obtained by the CLUSTER satellites. The data contains the upper triangle for the 5x5 correlation matrix of the three magnetic and two electric components of the electromagnetic field in 27 frequency bands in the SR2 reference frame. For more information, refer to http://caa.estec.esa.int/documents/UG/CAA_EST_UG_STA_v35.pdf
Creators: Pisa, D.
Publisher: iap.cz
Cassini RPWS/HFR Calibrated Jupiter Flyby Dataset Product Catalog
Creators: Baptiste Cecconi
Contributors: Philippe Zarka, PADC
Publisher: Paris Astronomical Data Centre - LESIA
EPN-TAP access to IAA-CAB-INTA-CSIC absorption cross sections database.
Creators: Jaime Jimenez
Publisher: Instituto de Astrofisica de Andalucia-CSIC; INTA-CAB
MCD is a database of atmospheric statistics compiled from Global Climate Model (GCM) numerical simulation of Martian atmosphere (http://www-mars.lmd.jussieu.fr). The GCM computes in 3D the atmospheric circulation and climate taking into account radiative transfer through the gaseous atmospheres and the dust and ice aerosols, includes a representation of the CO2 ice condensation and sublimation on the ground and in the atmosphere, simulates the water cycle (with modelling of cloud microphysics), the dust multisize particle transport, the atmospheric composition controlled by the photochemistry and the local non-condensible gas enrichment and depletion induced by CO2 condensation and sublimation, and has been extended into the thermosphere and to model ionospheric processes (due to chemistry). The database extends up to exobase (the top of the thermosphere, roughly at 300km in altitude); in addition to statistics on temperature, wind, pressure, radiative fluxes, it provides data such as atmospheric composition (including dust water vapor and ice content) and make use of 'dust and Extreme Ultra Violet (EUV) scenarios' to represent the variation of dust in the atmosphere and solar EUV conditions.
Creators: Zi Yin, Alexandre Rostaing
Contributors: Ehouarn Millour, Stéphane Erard, PADC
Publisher: LMD
The European Space Agency's Planetary Science Archive (PSA) is the central repository for all scientific and engineering data returned by ESA's Solar System missions, as well as several ground-based cometary observations. The EPN-TAP service provides links to zipped archives containing PDS data.
Creators: Angel Montero, Alan MacFarlane
Contributors: ESA / PSA
Publisher: European Space Agency
ExPRES Simulation service catalog
Creators: A. Loh
Contributors: B. Cecconi, PADC
Publisher: Paris Astronomical Data Centre - LESIA
VO-compliant and interactive encyclopaedia of extrasolar planets.
Creators: Jean Schneider
Contributors: PADC
Publisher: Paris Astronomical Data Centre - LUTH
Profiles of species in Venus atmophere terminator. Data retrieved from calibrated spectra obtained with the SPICAV-SOIR instrument on board the Venus Express spacecraft. These spectra can be checked on the ESA PSA repository. See: A.C. Vandaele et al., Contribution from SOIR/VEX to the updated Venus International Reference Atmosphere (VIRA), Adv. Space Res. (2015), http://dx.doi.org/10.1016/j.asr:2015.08.012.
Creators: Loic Trompet
Contributors: AC Vandaele, A Mahieux, V Wilquet, S Chamberlain
Publisher: BIRA-IASB
Mars-Express/High Resolution Stereo Camera (HRSC) panchromatic nadir images of planet Mars in radiometrically calibrated and orthorectified form, where the rectification is based on the terrain representation provided by the MOLA digital terrain model (HRSC processing level 3). This service provides links to separate services serving single images compliant to the Open Geospatial Consortium's Web Mapping Service (WMS). The original level 3 data in native PDS format is available online at https://archives.esac.esa.int and http://pds-geosciences.wustl.edu/missions/mars_express/hrsc.htm. The data has been re-projected to the Equidistant Cylindrical projection using the Mars sphere with radius R=3,396 km as its geodetic basis. Details about the HRSC experiment are described in Jaumann et al., 2007 (doi:10.1016/j.pss.2006.12.003).
Creators: Sebastian Walter
Publisher: Freie Universitaet Berlin
Solar active regions extracted from Heliophysics Feature Catalog.
Creators: Jean Aboudarham
Contributors: Xavier Bonnin, Christian Renié, PADC
Publisher: Paris Astronomical Data Centre - LESIA
Solar type 3 bursts extracted from Heliophysics Feature Catalog.
Creators: Jean Aboudarham
Contributors: Xavier Bonnin, Christian Renié, PADC
Publisher: Paris Astronomical Data Centre - LESIA
Hisaki/Exceed EUV Planetary observation database
Creators: Tomoki Kimura
Contributors: Atsushi Kumamoto, Pierre Le Sidaner, Baptiste Cecconi
Publisher: Tohoku University
IMPEx simulation runs provided by FMI, LATMOS and SINP
Creators: Tarek Al-Ubaidi
Contributors: IMPEx-FP7 Project Team
Publisher: IWF
Iitate Planetary Radio Telescope Data
Creators: Dr. Fuminori Tsuchiya
Contributors: Baptiste Cecconi
Publisher: Tohoku University
Measurements of comet Halley in the spectral channel of IKS on board the Vega-1 spacecraft. Data are retrieved from the PDS Small Bodies Node archive (2011 reformatted version) and completed with extra information from the original team. The dataset consists in 101 tables providing the calibrated radiance spectra of comet Halley as distance decreases, plus two composite spectra in different spectral ranges. For details and further references, see: Combes M. et al., 1988, The 2.3-12 micron Spectrum of Comet Halley from the IKS-VEGA Experiment, Icarus, 76, 404-436.
Creators: LESIA
Contributors: Stéphane Erard, IKI, PDS, PADC
Publisher: Paris Astronomical Data Centre - LESIA
Iitate log periodic Radio antenna High Resolution data
Creators: Dr. Atsushi Kumamoto
Contributors: Baptiste Cecconi, Pierre Le Sidaner
Publisher: Tohoku University
Illumination by the Sun of each face of the comet 67P/Churyumov-Gerasimenko based on the shape model CSHP_DV_130_01_LORES_OBJ.OBJ. The service provides the cosine between the normal of each face (in the same order as the faces defined in the shape model) and the Sun direction; both numerical values and images of the illumination are available. Each map is defined for a given position of the Sun in the frame of 67P (67P/C-G_CK). Longitude 0 is at the center of each map. The code is developed by A. Beth, Imperial College London, UK and the service is provided by CDPP (http://cdpp.eu). Acknowlegment: The illumination models have been developed at the Department of Physics at Imperial College London (UK) under the financial support of STFC grant of UK ST/N000692/1 and ESA contract 4000119035/16/ES/JD (Rosetta RPC-PIU). We would also like to warmly thank Bernhard Geiger (ESA) for his support in validating the 2D-illumination maps.
Creators: Arnaud Beth, Imperial College London, Dpt of Physics (firstname.lastname@example.com)
Contributors: CDPP, Nathanaël Jourdane, ESA, Stéphane Erard, Imperial College London, STFC/UK
Publisher: Centre de Données de la Physique des Plasmas (CDPP)
EPN-TAP access to the LOFAR JUPITER database.
Creators: Lukasz Tomasik
Publisher: Space Research Centre of Polish Academy of Sciences
Omega spectral cubes from PSUP. The database contains OMEGA observations acquired with the C (short wavelength NIR) channel. Filtering processes have been implemented to remove some instrumental artefacts and observational conditions. OMEGA C channel data cubes are corrected for atmospheric and aerosol contributions. Data are available as netcdf and idl sav files.
Creators: Karin Dassas
Contributors: IDOC
Publisher: Institut d'Astrophysique Spatiale - IDOC
Omega derived maps at PSUP. Mineralogical and albedo maps derived from OMEGA/Mars-Express observations, distributed as fits files.
Creators: Karin Dassas
Contributors: IDOC
Publisher: Institut d'Astrophysique Spatiale - IDOC
Compiled database for asteroid spectra in the visible and nir regions.
Creators: Mirel Birlan
Contributors: M. Popescu, Jonathan Normand, PADC
Publisher: Paris Astronomical Data Centre - IMCCE
A Transplanet model of magnetosphere-ionosphere coupling at Earth, Mars, and Jupiter
Creators: M. Indurain
Contributors: CDPP
Publisher: Centre de Données de la Physique des Plasmas (CDPP)
This service provides the most accurate values of dimensions, mass, and rotation period of solar system planets. These data are retrieved from Archinal et al 2018 (IAU report 2015, 2018CeMDA.130...22A) (radii) and Cox et al 2000 (Allen's astrophysical quantities, 2000asqu.book.....C) (masses, heliocentric distances, and rotation periods).
Creators: Stéphane Erard
Contributors: PADC
Publisher: Paris Astronomical Data Centre - LESIA
Catalogue of Martian impact craters with properties, from Robbins & Hynek 2011 (10.1029/2011JE003967)
Creators: Mikhail Minin
Publisher: Jacobs Uni
The ephemeris were produced by simulating the ejection of meteoroids from the sunlit hemisphere of cometary nuclei, typically from 0 to 3 au, followed by the propagation of orbits of meteoroids in the Solar System, taking into account the gravitation of the Sun, the 8 planets, Pluto, and the Moon, as well as the radiation pressure and the Poynting-Robertson drag. Note that asteroid parent bodies were considered as active (i.e. comet-like bodies) even if they are not active today. The showers are predicted when a planet enters a large enough set of meteoroids, at a distance less than typically 0.01 au. See Vaubaillon J., Colas F., Jorda L. 2005 A new method to predict meteor showers. I. Description of the model, Astronomy and Astrophysics, Volume 439/2 p.751-760, as well as: Vaubaillon J. 2017 A confidence index for forecasting of meteor showers, Planetary and Space Science, Volume 143 p.78-82
Creators: Jeremy Vaubaillon
Contributors: PADC
Publisher: Paris Astronomical Data Centre - IMCCE
The EPN-TAP 2.0 version of the complete asteroid data from the Minor Planet Center (MPC), updated once per month. The MPC operates at the Smithsonian Astrophysical Observatory under the auspices of Division III of the International Astronomical Union (IAU). The MPC Orbit database contains orbital elements of minor planets that have been published in the Minor Planet Circulars, the Minor Planet Orbit Supplement and the Minor Planet Electronic Circulars..
Creators: Williams, G., Keys, S., Rudenko, M., Galache
Publisher: The GAVO DC team
This service provides metadata information and hyperlinks to a subset of the M3/Chandrayaan-1 spectral cubes dataset provided by the PlanetServer/EarthServer-2 project as OGC/WCS endpoints. The data here hyperlinked is a subset of the original archive, composed by M3 L2 data, re-projected using the ISIS software to suit the interactive interface provided by the PlanetServer (http://access.planetserver.eu/) as described in Marco Figueira et al, 2018 (https://doi.org/10.1016/j.pss.2017.09.007). The original dataset is described in Pieters et al., 2009 (https://www.jstor.org/stable/24105459), and is distributed in native format on the PDS Geosciences node and ISRO Science Data Archive, https://pds-imaging.jpl.nasa.gov/volumes/m3.html.
Creators: Mikhail Minin
Contributors: C. Brandt, A. P. Rossi
Publisher: Jacobs Uni
The Cosmic Dust Catalog Volume 15 main page: http://curator.jsc.nasa.gov/dust/cdcat15/ParticleList.cfm and The Cosmic Dust Catalog Volume 15 explanation guide: http://curator.jsc.nasa.gov/dust/cdcat15/index.cfm, The Cosmic Dust Catalog Volume 18 main page: http://curator.jsc.nasa.gov/dust/cdcat18/index.cfm The service also provides a digitalized spectrum data derived by the Cosmic Dust Catalog Volume 15. The method of digitization is described by Lasue et al. 2010 Automated classification of interplanetary dust particles: Johnson Space Center Cosmic Dust Catalog Volume 15; doi:http://onlinelibrary.wiley.com/doi/10.1111/j.1945-5100.2010.01059.x/full. The digitalized spectra files in the service are provided courtesy of J. Lasue
Creators: IA2
Contributors: INAF-IAPS
Publisher: IA2
Dynamic Spectra of the Routine observation of Jupiter with the Nancay Decameter Array. This dataset contains two series of dynamic spectra recorded on each of the Nançay decameter sub-arrays (i.e. on Left Hand and Right Hand Polarization). The receiver is sampling from 10 MHz to 40 MHz with 75 kHz steps on the spectral axis. It records one spectrum every second on each polarization. The list of observation frequencies is provided.
Creators: Baptiste Cecconi
Contributors: Andrée Coffre, Emmanuel Thétas, PADC
Publisher: Station de Radioastronomie de Nançay (SRN)
This service is a redesigned version of the PDS spectral library, with data files provided as VOtable. The native version is distributed by the PDS Geosciences node: http://pds-geosciences.wustl.edu/mro/mro-m-crism-4-speclib-v1/mrocr_90xx/ Reference: Murchie et al (2007) Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on Mars Reconnaissance Orbiter (MRO). JGR Planets, 112:E05S03
Creators: Stéphane Erard
Contributors: PADC
Publisher: Paris Astronomical Data Centre - LESIA
Images, maps, photometries and other kind of planetary graphic platforms made by amateur astronomers. Data is received by the astronomers themselves and can be subject of change.
Creators: Jon Juaristi-Campillo
Contributors: Ricardo Hueso
Publisher: Euskal Herriko Unibertsitatea, Universidad del Pais Vasco, University of the Basque Country
Planetary and heliophysics plasma data at CDPP/AMDA
Creators: Centre de Données de la Physique des Plasmas
Publisher: Centre de Données de la Physique des Plasmas
HST observations of planets, dwarf planets, and satellites, extracted from the CADC database catalogue (regularly updated). Data are linked to the CADC repository, with file names common to all HST archives. Both calibrated and derived products are included. The main target is identified. Physical ephemeris and thumbnails are provided when available. Files and previews are not accessible during the proprietary period.
Creators: Stéphane Erard
Contributors: PADC, CADC
Publisher: Paris Astronomical Data Centre - LESIA
RadioJOVE Data Archive
Creators: Baptiste Cecconi
Contributors: Renaud Savalle, PADC
Publisher: LESIA
SPICAM/Mars-Express: Vertical profiles of temperature, CO2, O3, and aerosols density derived from UV occultations. Maattanen et al 2013 (2013Icar..223..892M)
Creators: Zi Yin, Alexandre Rostaing
Contributors: Anni Määtänen, François Forget, Sébastien Lebonnois
Publisher: LATMOS
SSHADE is an infrastructure for Solid Spectroscopy hosting a set of specialized databases provided by several research groups. SSHADE distributes spectral and photometric data (transmission, reflectance, optical constants, Raman, etc) obtained by various spectroscopic techniques over the whole electromagnetic spectrum but mostly covering the X, UV, Vis, Near/Mid/Far-IR, and sub-mm ranges. The measured samples include ices, minerals, rocks, organic, carbonaceous materials, and liquids — including field samples, synthesized and extraterrestrial materials. A dedicated search/visualization/export interface is available at https://www.sshade.eu. Information on SSHADE and its databases can be found at https://wiki.sshade.eu/
Creators: Damien Albert, Philippe Bollard
Contributors: IPAG/CNRS, SSHADE partners, Bernard Schmitt
Publisher: OSUG Data Center
This service provides a compilation of global spectra of planets and satellites in the visible and NIR range, for quick reference purpose. Spectra are selected from various libraries, including the Tohoku-Hiroshima-Nagoya Planet Spectra Library (Lundock et al 2009) and a USGS web site (R. Clark). Reformatted VOtable versions are provided together with links to the original data.
Creators: Stéphane Erard
Contributors: PADC
Publisher: Paris Astronomical Data Centre - LESIA
This service publishes spectral matrix data from the Earth magnetosphere obtained by the THEMIS satellites. The data contains the upper triangle for the 6x6 correlation matrix of the three magnetic and three electric components of the electromagnetic field in 164 frequency bands in the magnetic field-aligned reference frame. For more information, refer to https://doi.org/10.1007/s10712-018-9496-9
Creators: Pisa, D.
Publisher: iap.cz
This service lists TNO thermal properties as derived mostly from Spitzer and Herschel observations
Creators: Emmanuel Lellouch, Florence HENRY
Contributors: PADC
Publisher: Paris Astronomical Data Centre - LESIA
Since 1973, the 18-cm lines of the OH radical have been systematically observed in a number of comets with the Nançay radio telescope. This allowed an evaluation of the cometary water… production rates and their evolution with time, as well as a study of several physical processes: the excitation mechanisms of the OH radio lines, the expansion of the cometary atmospheres, their anisotropy in relation with non-gravitational forces, the Zeeman effect in relation with the cometary magnetic field. The Nançay observations of 53 cometary apparitions between 1982 and 2009 are now organized in this database.
Creators: Jacques Crovisier
Contributors: Mathieu Hirtzig, PADC
Publisher: Paris Astronomical Data Centre - LESIA
UCL Magnetodisc Model for Jupiter and Saturn. The data consists of the magnetic field in JMAG spherical coordinates. For details and further references, see: Achilleos N. A., Guio, P. and Arridge, C. S., 2010, A model of force balance in Saturn's magnetodisc, MNRAS, 401, 2349-2371 [2010MNRAS.401.2349A]
Creators: Patrick Guio, UCL (firstname.lastname@example.com)
Contributors: Nick Achilleos, Patrick Guio
Publisher: University College London
USGS planetary maps are accessible through WMS queries and can be displayed in QGIS or similar software. The original archive is located at https://astrogeology.usgs.gov/maps
Creators: Mikhail Minin
Publisher: Jacobs Uni
The service provides access to the complete dataset of VIMS spectral cubes on Saturn's moons illustrated by multispectral previews. It is linked to the web site at Laboratoire de Géologie Planétaire, Nantes (https://vims.univ-nantes.fr) which contains more information about observing sessions. Raw VIMS cubes are available (PDS format), as well as calibrated and geometry files (both in ISIS format). See Le Mouelic et al (2019) Icarus 319, 121-132. The original archive is distributed on the PDS imaging node (https://pds-imaging.jpl.nasa.gov/volumes/vims.html)
Creators: Benoit Seignovert, Stephane Le Mouelic, Christophe Sotin
Contributors: LPG, ObsParis
Publisher: ObsParis
VIRTIS/Venus Express demonstrator service: imaging spectroscopy of Venus in the visible and the near infrared. This lists all the calibrated files from the nominal mission for the three channels M-vis, M-IR and H. Files are described according to the extended index in the PSA archive, with links to the PSA: ftp://psa.esac.esa.int/pub/mirror/VENUS-EXPRESS/VIRTIS/VEX-V-VIRTIS-2-3-V3.0/. See Piccioni et al, 2007, VIRTIS: The Visible and Infrared Thermal Imaging Spectrometer, ESA SP 1295.
Creators: Stéphane Erard
Contributors: Florence Henry, PADC
Publisher: LESIA
Venus-Express Observations of the Magnetic Field in VSO Coordinates including Spacecraft Positions
Creators: Al-Ubaidi, Tarek, Scherf, Manuel, Zhang, T.
Publisher: IWF
This database displays vertical profiles of temperature and composition in Titan's atmosphere at nine different latitudes between 100 and 500 km. These profiles were retrieved from the infrared spectra acquired by the Composite Infrared Spectrometer (CIRS) aboard the Cassini spacecraft. The retrieval method and the description of the used dataset is detailed by Vinatier et al., 2009, Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission. I: Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles, Icarus, in press. doi:10.1016/j.icarus.2009.08.013.
Creators: Sandrine Vinatier
Contributors: PADC
Publisher: Paris Astronomical Data Centre - LESIA
Voyager PRA (Planetary Radio Astronomy) Datasets catalog. The dataset are originally published by several data centers: NASA/PDS, NASA/NSSDC, NASA/GSFC, Univ. Iowa and CNES/SERAD.
Creators: Baptiste Cecconi
Publisher: Paris Astronomical Data Centre
Solar survey archive Bass2000.
Creators: Jean Aboudarham
Contributors: Christian Renié, PADC
Publisher: Paris Astronomical Data Centre - LESIA
The data provided by PlanetServer are higher-order products derived from a subset of the complete CRISM dataset (http://crism.jhuapl.edu/). For the original CRISM dataset (Murchie et al., 2007, https://doi.org/10.1029/2006JE002682), please visit PDS Geosciences node, https://pds-geosciences.wustl.edu/missions/mro/crism.htm. This service provides metadata information and access-URLs to the PlanetServer data access OGC/OWS endpoints as well as hyperlinks to access the interactive interface provided by the service. The data provided by PlanetServer was atmospherically calibrated and geo-referenced as described in Figueira et al., 2018 (https://doi.org/10.1016/j.pss.2017.09.007). For the interactive interface, go to http://access.planetserver.eu
Creators: Mikhail Minin
Contributors: C. Brandt, A. P. Rossi
Publisher: Jacobs Uni
SELECT * FROM ... WHERE (1 = ivo_hashlist_has(lower("target_name"),lower('Saturn')) OR 1 = ivo_hashlist_has(lower("target_name"),lower('6')) OR 1 = ivo_hashlist_has(lower("target_name"),lower('699'))) AND time_max <= 2456018.50000000 AND time_min >= 2455987.50000000
PDAP Resources (by dataset)
NASA PDS Query
- https://pds.nasa.gov/services/search/search?q=target%3ASaturn+AND+%28start-time%3A%5B0001-01-01T00%3A00%3A00Z+TO+2012-04-01T00%3A00%3A00Z%5D+AND+stop-time%3A%5B2012-03-01T00%3A00%3A00Z+TO+9999-12-31T23%3A59%3A59.999999Z%5D%29


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applying veneer to safe room door4/26
I am a cabinet and trim man. I have a job going that they told me after I had started that they wanted me to cover a metal storm room door with wood. I had heard you could use contact cement, and have used it in the past for formica, so thought no problem. I put my veneer on, and thought all was good. a few days later, there were bubbles. I tried to hammer them out, and to weight them down to get it to adhere, but it still would bubble up. I have now purchased a second veneer, and partially removed the first one. In the worst bubble, it looks as if it pulled paint off the door, but the others just look as if they did not stick. Has anyone done what I am trying to do? is contact cement the right thing, or is there a better glue to use? Thanks for any help!
If they want it to look like wood, use wood. Real wood. There is no reason to not use real wood for this door. We have even made wood doors that are bulletproof.
I would try a Phenolic backed veneer. If you are not familiar with this, it is a laminate sheet with a thin veneer applied to it. It will take you a few weeks to get. Contact adhesive is really your only choice.
Bubbles in a veneer usually means you did not let the vapors escape. Assuming there is no chips or debris under the veneer. I have used contact adhesive on wood veneers. The problem with the metal door is that the steel and the wood will expand differently.
Did you use water based contact cement?
We use only flammable adhesives.
In the late 80's and early 90's, WilsonArt came out with a non-flammable adhesive and we used that for a while. About 18 months after the installation, we began to get lifting of the laminate. It was a common problem with everyone that used this glue. We called it The Blue Flu because it was blue in color.
Eventually, WilsonArt helped with some re-reimbursement for re-work, but we did not come out whole. Since then, we only use flammable adhesives.
The reason I asked was because the solvent based is probably acting like a paint stripper on the painted door. Surprised the whole sheet of veneer didn't fall off.
Rich C.
You might be right. He should have noticed that, if the paint was dissolving. He will find out now, he will have to strip the door if he is going to put on another veneer.
I did use a solvent based. In the worst bubble the paint did pull loose. The rest of it seemed stable. But I am considering sanding all the paint off the metal, and trying it again, unless someone can see a obstacle that direction. Thanks for the help so far.
I used to work for a commercial door manufacturer that regularly applied two ply (mdf core & wood veneer) door skins to metal doors. If I remember correctly they used a "reactive hot-melt" adhesive that was developed specifically for that application (wood to metal). I do know it took multiple tries to get it "right" and even then there were occasional failures.
I also remember one thing; if the adhesive had any water in it, the steel door "core" would develop a light coat of rust, and nothing stayed stuck to it for long. Stay away from water-based adhesives.
I don't think that contact cement (including solvent-based) has any real chance of success either. I think you need to go with one of the new "high tech" adhesives to have a chance at getting a lasting bond.
You can do it with two adhesives we've used for this exact thing in the past. Polyurethane (Gorilla Glue) and thickened epoxy assuming you're using either a paper backed or two ply wood veneer. Definitely sand off all the paint and scuff the door hard with some coarse 36 grit or so sandpaper as both adhesives are making mechanical bonds to the metal. The Poly should be done in a vacuum bag but the thickened epoxy could be done on site. Use a notched trowel to get an even pattern of epoxy lines over the entire door and press your veneer skin down into the epoxy. Use a hardwood block to rub over the entire surface much like hammer veneering but without so much pressure. The goal is to even out the epoxy and uniformly press the veneer down.
I used an adhesive from Spectrum that was designed for metal to wood. It did require clamping by vacuum or other press.
This sounds like an excellent opportunity to have a faux finisher come in and paint it to look like the wood of their choice, without future veneer/steel/glue incompatibility issues.


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Cosmo Jarvis played a wonderful acoustic set last evening in the idyllic surrounds of the iconic Pure Pop Courtyard to a rapt crowd that spilled into the record store itself and the street beyond. All the way from the UK, it seemed a pity that Cosmo was only playing this one show in Melbourne, but thankfully he will be returning in December with his band to play more venues, and given his performance at Pure Pop it's not hard to see most of the audience returning to see him again.
Tag Archives: davy simonyContinue reading
Cosmo Jarvis @ Pure Pop Records, 3rd Of August


text: CHEAT SHEETTOP 10 RIGHT NOWPopularRihanna Beats Gaga for Most Facebook LikesUpdated 04.24.17 3:16PM ET / Published 07.15.11 12:27PM ET Richard Drew / AP PhotoMaybe Gaga can go to Google+: Rihanna took the lead in Facebook fans, edging out Gaga's 40,544,276 with 40,566,359. She updated her status to "40 mil! 1 LOVE #RihannaNavy." Gaga, however, still reigns supreme on Twitter, with more than 11 million fans, and she's the most-viewed YouTube star despite being banned. Rihanna has 6 million Twitter followers and is the third-most-viewed person on YouTube.Read it at E! Online


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Our round up of staff picks from the wide world of Indie music. This edition we feature Tomberlin - At Weddings, Wire reissues, Tony Molina - Kill The Lights, Ty Segall & White Fence - Joy, Thee Oh Sees - Smote Reverser, and the Moldy Peaches - S/T.
In our latest First, Last, and Favorite column we get some light shed on the the influences behind Seattle trio Weep Wave's 'S.A.D.'
We get to know NW punks Sleepover Club through the records they love! W(PH)OOPSIE their latest record is out next week!!
Julia Shapiro shares thoughts on a few of her favorite records. She's performing live in our shop this Thursday with her new record Perfect Vision available as well!
We learn a little more about the listening lives of Tacocat, from first CDs to current obsessions. Get excited for the release of their new record 'This Mess Is A Place' out this Friday from Sub Pop!
Our expert staff shares a few of the RSD 2019 releases they're most excited for. Time to update your wantlist!


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Alesha MacPhail murder – Monster Aaron Campbell's legal fees to cost taxpayer more than £100,000 after sentence appeal granted
The fiend was sentenced to 27 years behind bars after the sickening murder and rape of the six-year-old last July
MONSTER Aaron Campbell's legal fees to appeal his life sentence will cost taxpayers more than £100,000, according to reports.
The fiend was sentenced to 27 years behind bars after the heinous abduction, rape and murder of tiny Alesha MacPhail, six, last year.
Campbell's legal costs have already surpassed a whopping £81,000 - a bill that was sent by the Scottish Legal Aid Board last week.
But after the lad - who turned 17 in a prison cell - was granted the right to appeal his minimum term, The Daily Record reports that the fees are set to soar beyond the £100k mark.
A SLAB spokesman told the publication: "Legal aid is paid directly to lawyers to represent people accused of serious crimes, including those viewed as being of an abhorrent nature, to help ensure a jury can reach an appropriate verdict in a timely manner.
"Serious cases such as this can result in higher payments to solicitors and counsel because of the nature of the charges and the amount and type of work this entails for their legal representation."
Campbell's hearing will take place on August 7 before three judges.
We told recently how Alesha's furious great-granddad blasted the decision to allow Campbell to appeal his sentence - insisting he'd "torture him himself".
A jury found Campbell guilty of the sickening murder of little Alesha and Lord Matthews sentenced him in March.
During his sentencing, Lord Matthews took into consideration Campbell's "arrogance and callousness".
He described his shock at seeing a police officer "break down in the witness box" for the first time in his career in court.
Alesha MacPhail murder: Aaron Campbell granted appeal against life sentence
Quotes from Campbell in his admission read that "all he thought about was killing her.
"That it was a moment of opportunity - at any other time in life murder would not have been the conclusion."
Vile Campbell finally admitted guilt earlier this morning of the heinous crimes.
The monster had blamed the crimes on dad Robert MacPhail's girlfriend, Toni McLachlan - claiming she "brutalised" the little girl.
related stories
But Ms McLachlan wept in the dock after he admitted all crimes.
Campbell's defending QC told the court his client shows many traits on the "psychopath checklist".
Alesha's grieving mum Georgina has vowed to confront her daughter's killer behind bars.
We pay for your stories and videos! Do you have a story or video for The Scottish Sun? Email us at firstname.lastname@example.com or call 0141 420 5200


text: On 2015-04-16 15:32, Stefan Karlsson wrote: > On 2015-04-16 14:33, David Holmes wrote: >> Hi Stefan, >> >> trimming ... >> >> On 16/04/2015 10:07 PM, Stefan Karlsson wrote: >>> On 2015-04-16 04:23, David Holmes wrote: >>>> Second, more important question: have you examined how this attribute >>>> affects the ability to walk the stack? We have already seen issues on >>>> some platforms where library functions, like abort(), have the >>>> noreturn attribute and as a result the call is optimized in a way that >>>> prevents the stack from being walked - see eg: >>>> >>>> https://git.matricom.net/Firmware/bionic/commit/5f32207a3db0bea3ca1c7f4b2b563c11b895f276 >>>> >>>> >>>> >>>> though this: >>>> >>>> https://www.raspberrypi.org/forums/viewtopic.php?t=60540&p=451729 >>>> >>>> suggests that problem may have been addressed by the libc folk. But it >>>> still raises the question as to how our own noreturn functions will be >>>> handled and how they will affect stacktrace generation in hs_err logs >>>> or via gdb. >>> >>> I added a call to fatal(...) in the GC code. I get correct stacktraces >>> in gdb, but the stacktraces in the hs_err files are broken with >>> fastdebug and product builds: >> >> Which platforms? > > On Linux x86 and x86_64. > >> >>> Stack: [0x00007f12518d2000,0x00007f12519d3000], sp=0x00007f12519d0eb0, >>> free space=1019k >>> Native frames: (J=compiled Java code, j=interpreted, Vv=VM code, >>> C=native code) >>> V [libjvm.so+0x11db44a] VMError::report_and_die()+0x1ba >>> V [libjvm.so+0x7efb80] report_vm_error(char const*, int, char const*, >>> char const*)+0x90 >>> V [libjvm.so+0x7efc49] report_vm_error_noreturn(char const*, int, char >>> const*, char const*)+0x9 >>> V [libjvm.so+0x7efc63] >>> V [libjvm.so+0xfd7937] >>> V [libjvm.so+0xfeec51] >>> ... >> >> So what is the plan: try to get hs_err working again? Or file this >> under "well it seemed like a good idea"? ;-) > > I'm leaning towards "seemed like a good idea", unless someone has an > easy fix for these problems. I've been looking a bit at this. It's not the stack trace per se that is broken, but the decoding of the function names is not working for some of the callers of the noreturn functions. I tried this with report_fatal using -XX:ErrorHandlerTest=5 and got the following: 0x7fb71ccd98d0 <report_fatal>: push %rbp 0x7fb71ccd98d1 <report_fatal+1>: mov %rdx,%rcx 0x7fb71ccd98d4 <report_fatal+4>: lea 0x9b4b34(%rip),%rdx 0x7fb71ccd98db <report_fatal+11>: mov %rsp,%rbp 0x7fb71ccd98de <report_fatal+14>: callq 0x7fb71ccd98c0 0x7fb71ccd98e3: data16 data16 data16 nopw %cs:0x0(%rax,%rax,1) So the report_fatal frame has ...98e3 as its return address, but that is actually outside the function and this causes dladdr() to return NULL in dli_saddr and dli_sname. The JVM then attempts to decode using Decoder::decode but I wasn't able to follow that code to understand why that fails. The same appears to happen for the caller of report_fatal (controlled_crash in my case) but there I can't explain why dladdr returns NULL values there. After these two functions the rest of the stack trace appears to be correctly decoded. One approach could be to attempt to inject a "nop" at the end of functions which call a "noreturn" function. This would hopefully make the instruction after the call to the noreturn function part of the caller and would make symbol decoding work. /Mikael > > Thanks, > StefanK > >> >> Cheers, >> David >> >>> Thanks, >>> StefanK >>> >>> >>> >>>> >>>> Thanks, >>>> David >>>> >>>>> >>>>> Thanks, >>>>> StefanK >>>>> >>> >


text: You cannot capture packets prior to the event packet, usually. The exception is if the session data is being reassembled. If a specific stream is being saved for reassembly and an event packet comes along, all of the saved packets are logged. Otherwise, snort does not buffer up session data as would be needed to log packets prior to an event generating packet. Once a packet causes an event you can use event tagging to log the rest of the session. Paul Melson wrote: >I'm using one of my Snort sensors (v2.3.2 w/ flexresp) to monitor, among >other things, outbound e-mail traffic. Right now I am logging to a MySQL >database and can view the offending packet data on a per-alert basis. In >the case of e-mail traffic, packet captures of lengthy messages (say those >with MIME attachments) don't always include the message headers. > >I have been reading up on stream4 and stream4_reassemble, hoping that I can >force Snort to match on (and thus log) the entire "client" side conversation >to the database, but I'm not having any luck. Here are the preprocessor >lines from my snort.conf file: > >preprocessor stream4: enforce_state disable_evasion_alerts memcap 67108864 >preprocessor stream4_reassemble: clientonly, ports 25 > >Unfortunately, I still only get the packet with the offending string in the >database. Am I barking up the wrong tree here? > >Thanks, >PaulM > > > > > >------------------------------------------------------- >This SF.Net email is sponsored by: NEC IT Guy Games. >Get your fingers limbered up and give it your best shot. 4 great events, 4 >opportunities to win big! Highest score wins.NEC IT Guy Games. Play to >win an NEC 61 plasma display. Visit http://www.necitguy.com/?r=20 >_______________________________________________ >Snort-users mailing list >Snort-users at lists.sourceforge.net >Go to this URL to change user options or unsubscribe: >https://lists.sourceforge.net/lists/listinfo/snort-users >Snort-users list archive: >http://www.geocrawler.com/redir-sf.php3?list=snort-users > > >


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An algal bloom is a rapid increase or accumulation in the population of algae (typically microscopic) in a water system. Cyanobacteria blooms are often called blue-green algae. Algal blooms may occur in freshwater as well as marine environments. Typically, only one or a small number of phytoplankton species are involved, and some blooms may be recognized by discoloration of the water resulting from the high density of pigmented cells.
Since 'algae' is a broad term including organisms of widely varying sizes, growth rates and nutrient requirements, there is no officially recognized threshold level as to what is defined as a bloom. For some species, algae can be considered to be blooming at concentrations reaching millions of cells per milliliter, while others form blooms of tens of thousands of cells per liter. The photosynthetic pigments in the algal cells determine the color of the algal bloom, and are thus often a greenish color, but they can also be a wide variety of other colors such as yellow, brown or red, depending on the species of algae and the type of pigments contained therein.


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The Trilogy 11:04
We Are The West Los Angeles, California
From beyond the setting sun comes the sound of We Are The West. The intrepid imaginers lay claim to no particular state or border, only a direction, calling the listener to explore the familiar and embrace the unknown. Their boldest vision yet is a portrait of endless possibility and sonic adventure that must be heard to be seen. We Are The West welcomes you to The Golden Shore. ... more
Streaming and Download help
If you like We Are The West, you may also like:
Bandcamp Daily your guide to the world of Bandcamp


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HYANNIS — The Lyndon Paul Lorusso Charitable Foundation and Grand Cove Productions will present the educational documentary "Not Yet" at 7 p.m. Thursday at the Barnstable Performing Arts Center.
"Not Yet" is a 30-minute film that includes interviews with inmates at the Barnstable County Correctional Facility and young people who have become addicted to opiates. It educates parents and teens on the dangers of prescription pain pills and how these pills lead to heroin.
One of the young women in the film, Rebecca, will take part in a panel discussion afterward, according to an announcement from the Barnstable Youth Commission.
Although the film contains graphic content, it is designed to be viewed by anyone age 13 or over. The event is free.
The panel discussion also will include Barnstable Police Chief Paul MacDonald, Barnstable County Sheriff James Cummings, "Not Yet" director-writer Thomas Milkey and Patricia Mitrokostas of Gosnold on Cape Cod. Anne Colwell, CEO of Cape Cod Child Development, will serve as moderator.
The performing arts center is at Barnstable High School, 744 W. Main St.
— K.C. Myers


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Valentine's Day BINGO
Do you need a fun way to celebrate Valentine's Day? BINGO is a great way to celebrate in your classroom.
These BINGO boards are differentiated to meet the needs of many learners k-5th grade or ability level.
Included are 4 different board levels ranging from quick play to long play. Each level includes 5 BINGO boards, enough for most small group sessions. If you have more students, simply print out more boards and let some kids play with the same board. They still have fun and they enjoy seeing who gets a BINGO at the same time!
*Each BINGO Set Has Color Coordinated Cards To Boards(Black, Red, Pink, Purple) So You Never Have To Worry About Using The Wrong Cards With Your Board Of Choice*
Included Please Find:
Call Cards For Quick Play 4x4
5 4x4 Quick BINGO Boards
Call Cards For Long Play 4x4
5 4x4 Long BINGO Boards
Call Cards For Quick Play 3x3
5 3x3 Quick BINGO Boards
Call Cards For Long Play 3x3
5 3x3 Long BINGO Boards
9 BINGO Call Out Cards: Valentine's Day Words
Thank You
Clip Art Credit


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There is one item matching your search.
ConnecticutUnited States. CT. North Windham, CT. Windham Co. (open 1838+). Dated 1912/02/24. Fine duplex ties 1c on ppc.Cover #81739 | Price: $10.00Add To Cart
Phil Bansner, Professional Philatelist
PO Box 6854 • Wyomissing, PA 19610
Phone (610) 678-5808 • Email email@example.com
Website design and programming by BB Design.


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As a beginner, it's fine even if you don't know how to tune the guitar manually. There are many Guitar tuning gadgets and software available. I would suggest not to waste your money in purchasing any tuning gadget. I have come across a software called "Digital Guitar Tuner" which I think is the best for tuning your guitar. It's a free software and very easy to use as well. You can tune your guitar within few minutes using this software. I myself use the same to tune my guitar and believe me, it's the best. Here's the link to download it:
Also, there are many other locations as well from where you can download 'Digital Guitar Tuner' for free.
Tuning your guitar within minutes
Subscribe to: Posts (Atom)


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Please select the district you are a coordinator for. As a coordinator you will be able to view all of your districts students, projects and make changes to them.
Attention Historical Papers and Website Contestants: Your projects must be completed and submitted by February 28th at 10:00 pm. (Exhibits, Documentaries, and Performances are due at the contest.)
UTVRHD 215 Estate Drive, Alpine, UT 84004
Competition Schedule
8:00-8:45am Student Check In & Exhibit Setup
9:00am-2:30pm Judging
4:00-5:00pm Awards Ceremony
* This schedule is subject to change.
Special Awards
As part of the centennial recognition of World War I, the Utah WWI Commission is sponsoring cash prizes for outstanding History Day projects relating to the Great War. Winners will be selected at Utah's ten regional History Day competitions held in February-March, as well as at the state contest held in April.
Projects must relate directly to World War I and may range from the war in Europe to its impacts on the home front, such as rationing, mining, industry, Liberty Bond drives, German POWs, conscientious objectors, politics, etc. Winning projects will demonstrate research, clarity, thought, and some originality. Relevant projects from all categories (documentary, paper, website, exhibit, and performance) will be considered.
The American Revolution Prize
The Colonial Heritage Foundation of Utah is a non-profit corporation dedicated to the preservation of the values, culture, skills and history of America's founding. The Colonial Heritage Foundation of Utah is sponsoring cash prizes for outstanding History Day projects relating to the American Revolution.
Projects must relate directly to the American Revolution and winning projects will demonstrate research, clarity, thought, and some originality. Relevant projects from all categories (documentary, paper, website, exhibit, and performance) will be considered.
Chaperone Policy:
Day of Contest Food Service Options:
Highland, Utah approxamately 2 miles South from Timberline Middle School has several restaurant options including, Wendy's, Little Caesar's and Domino's Pizza, Taco Time, Subway, Roxberry Juice and Pizza Pie Cafe. Additionally, Ridley's and Meiers Meat and Fine Foods also provide deli service food options. No food service will be provided at the contest location.
Contact Us:
Thanks for participating in Utah History Day 2019. We are excited to learn more about you and your historical projects.
For information about the contest (where, when, time, directions, etc.) click on the General tab.
To update your profile, click on your name (above right). Keep your username and password in a safe place. Use the Login option (top right) to access the system after you have registered.
If you have questions about your registration, please send an email to firstname.lastname@example.com.
Students (except website and historical papers) please check to make sure you have four copies of your process paper and bibliography with you!
At 9:00 am, judging starts in all categories. All exhibits must be completely set up in the gym before 9:00am as the doors to the gym will be closed to public viewing from 9:00- 10:00am and from 12:00-1:00pm.
Students with documentaries should know that the room is set for standard HDMI and VGA connections. If the student's tech that is being used to play their documentary is newer than these connections, they need to bring their own adapter. We strongly recommend students bring a laptop to show their documentary. Students with documentaries should make sure that all their current computer programs (software) and operation updates on their laptops are current.
Occasionally in the rooms showing documentaries, individuals have run into trouble with technology and interface set up because recent updates have not been done on their end. Schools frequently update their IT systems and difficulties have occurred in the past that can be easily avoided. All students showing documentaries should be prepared to be completely IT self-sufficient in their presentations. Judges will not be able to assist students with IT problems
Here are some general guidlines about our expecatations for the regional contest:
Thank you for helping your students participate in Utah History Day 2019!
Teachers must register themselves before students can register. To get started, click on the Register tab above, then select Teacher.
You can view your students' registration information under My Students.
To update your profile, click on your name (above right). Keep your username and password in a safe place. Use the Login option (top right) to access the system after you have registered.
Below is some general information regarding the regional contest:
To sign up as a contest judge for the Utah Valley Regional contest, please select "create account" along the top white bar of this webpage, and select "judge" from the drop down menu options. This will take you through the process of completing your judges profile.
If you have already registered as a contest judge, you will receive details about your judging assignment via email in the near future. We are grateful for your service and look forward to working with you this year.
If you have any questions, please contact:
Amy Thackeray
Email: email@example.com
Phone: 801-427-7441
Website: Utah History Day


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Contact Us
Seapoint Canoe Centre is located adjacent to a Pay & Display car park. Metred parking is also available on Prince's Parade which is free from October - March. Blue badge car spaces are available in the car park.
Access to the canal is directly behind Seapoint Canoe Centre. After collecting your canoe or kayak you would carry it down a grassy bank to the pontoon on the canal, approximately 10 metres behind the centre.
Directions By Car
From Folkestone, follow Sandgate Road towards Hythe, turn left just before the garage near Seabrook, drive along Prince's Parade on the seafront and take the first turn on the right signposted "P" for parking, our Seapoint sign is at the entrance of this turning. A Pay & Display car park is adjacent to the centre.
From Hythe turn right into Twiss Road, follow the road round onto Prince's Parade, past Hotel Imperial on your left and continue along the seafront to the far end. Turn left at the "P" for parking. A Pay & Display car park is adjacent to the centre.
From London and/or the M25, take the M20 towards Folkestone. Take Junction 11 (A261) to Hythe. When in Hythe, follow signs in the direction of Folkestone. Turn right into Twiss Road opposite the Bell Inn, follow the road onto Prince's Parade on the seafront, continue past Hotel Imperial and its golf course. Seapoint Centre is towards the end of the Parade. Turn left at the "P" for parking , the pay & display carpark is adjacent to the centre.
Direction By Train from London
55 minutes from London St Pancras to Folkestone, then cycle or take a taxi to the centre down on the coast:
Folkestone West Train Station is 2.4 miles from Seapoint Canoe Centre.
Folkestone Central Train Station is 2.9 miles from Seapoint Canoe Centre.


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2 injured in Lyndhurst firePosted: Updated:
Two people were injured in an early morning fire in Lyndhurst.
A fire official says an off-duty officer smelled smoke in the area of 518 Willow Ave. at around 4 a.m.
Two people inside the house climbed onto the roof and fire crews used a ladder to rescue them.
Both people were taken to the hospital and are in stable condition.
Fire officials say there were no smoke alarms in the home. They say the fire severely damaged the basement and first floor of the house.
The cause is under investigation.


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Here you will learn your boats maximum height, draft, and beam, and minimum fuel range, as well as what to expect along the way. After months of excitedly preparing your boat and yourself for your dream trip, the next step is getting familiar with each leg of this amazing . Every year around a hundred boats prove this point by completing a circumnavigation of the entire eastern U. Enjoy and happy cruising. Loopers," as they are often . This is the best of the best!
John took his BEST SELLER and made it extraordinarily better. It includes everything you need to know to cruise the . ChartKit Region Block Islan R. LIVRE: par CAROLE DUVAL. Great Loop Passage Planner.
You know what general direction the bathroom is in, but the trip seems daunting. Therefore we have put this report together as an introductory guide . Looking for the cruise of a lifetime?
The degree is given in recognition of completing. The aptly named loop is a route. It turned out, he did it sooner, and sooner in life than any other solo sailor on record who . Jerry is a frequent speaker at AGLCA rendezvous. Midlan Ontario to Mobile Alabama on their foot sailboat Adamant 1. The major expense of which, always boils down to your own individual lifestyle, boating philosophy, . Starting in his home town TK outside of Cincinnati, Tart would paddle . Worried about what it might cost?
Featuring… Lighthouses. The waterway stretches from the Florida Keys to Canada, and connects rivers with the Atlantic Intracoastal Waterway. The dissertation explores the operative function of incompletenesses in occidental symbolic systems that work with discrete alphabets. However, the starting point for the analysis is the transmission of mathematical and metamathematical knowledge between China and Europe – between an incomplete . Lynn Seldon, Boating Writer. Map used with permission Raven Cove Publishing.
Whether planning the trip of a lifetime encompassing the entire route (up to 3miles) or just boating a portion of this classic . The beauty of the concept is that it takes on many different variations and side- trips depending on the starting and ending point, and the particular interests and. Our trip will take us away from South Dakota for one year as we travel 0to 0miles on our Rangertugboat.
We will celebrated years of married life so we figure we can stand the close quarters as we adventure together. What could possibly go wrong? We will try to keep the map updated so you can see our progress and see photos along the way. We could have followed the Erie Canal all the way to Buffalo and into Lake Erie, but we decided to see what Canada had to offer with the Trent-Severn .


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iOS Software Development Engineer - IMDb
Seattle (King) Design / Civil engineering / Industrial engineering
Job description
IMDb is the world's most popular source for everything about movies & TV with over 250 million unique monthly visitors and 50 million iOS app downloads on the App Store. We are looking for a software development engineer to join our iOS Development Team and lead the effort of building the next generation of our hugely popular iOS app "IMDb Movies & TV", currently rated 5-stars on the App Store.
IMDb sits at the intersection of the entertainment, media, and technology markets inside the world's most innovative and consumer-centric company – Amazon.com. As a software development engineer at IMDb, you will have the opportunity to learn and use Amazon technologies from all over the company to build amazing products, which will be used directly by fans and movie & TV industry professionals. IMDb employees enjoy the benefits of working for Amazon with the autonomy of working on a small, nimble team, with people who love movies & TV (from Hitchcock to Batman Begins, from Gilmore Girls to Archer and Transparent).
The IMDb iOS app is built on top of the latest iOS and open-source frameworks, as well as Amazon cloud computing technologies based on AWS. In order to serve our iOS customers around the world with the most up-to-date entertainment information, you will work closely with product owners, designers, and other developers to build engaging and personalized user experiences, and to deliver improvements to performance, reliability, and security.
Join us if you are a movie and TV fan, want to grow your career, learn new technologies and skills, and make an impact on products used by millions every day!
Amazon is an Equal Opportunity-Affirmative Action Employer - Minority/Female/Disability/Vet
Ideal candidate profile
· 1+ years of professional software development experience.
· Programming experience with at least one modern
· language such as Java, C++, or C# including object-oriented design.
· 1+ years of experience contributing to the architecture and design (architecture, design patterns, reliability and scaling) of new and current systems.


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Location, location, location! 6 acres m/l on the corner of Hwy 6 & Hwy 129 in Green City. Approximately 300 yards of Highway 6 frontage. The perfect high traffic location for your business. Call Erica Supple at 660-988-0149 for your showing!
The seller has not posted any comments at this time.
No one has commented on this property at this time.
No Open Houses scheduled at this time.
Mortgage information currently not available.