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Welcome to the Delaware Small Business Chamber!
We are an independent Delaware chamber of commerce supporting small businesses throughout the State of Delaware and the surrounding business communities. Our focus is on businesses with 0 to 100 employees and any business that economically supports our local small business community.
Tax Reform Lunch-n-Learn
DSBC Tax Reform Seminar
Date: January 15, 2020
Time: 11:30 AM – 1:00 PM EST
Location: DSBC Office – 11F Liberty Plaza, Newark, DE 19711
SMART Lunch-n-Learn
Tax-Free Retirement Seminar
Taxes, Income & Retirement
Date: January 23, 2020
Time: 11:30 AM – 1:30 PM EST
Location: DSBC Office – 11F Liberty Plaza, Newark, DE 19711
Bagels & Benefits
Get to know the DSBC and their benefits!
Join us for FREE bagels and coffee
Date: January 29, 2020
Time: 9:00 AM – 11:00 AM EST
Location: DSBC Office – 11F Liberty Plaza, Newark, DE 19711
60 Second Networking
DSBC 60 Second Networking in Georgetown
Meet 15 other business professionals in less than two hours!
Date: February 4, 2020
Time: 2:30 PM – 3:45 PM EST
Location: Georgetown Arena's – 21553 Rudder Lane, Georgetown, DE. 19947
(private room to the left)
Women on the R.I.S.E.
Delaware Small Business Chamber's Women's Networking Series
This is one Women on the R.I.S.E. you will not want to miss!
Date: February 13, 2019
Time: 4:00 PM – 6:00 PM EST
Location: TBD North Wilmington
Lunchtime Mixer Texas Roadhouse
Delaware Small Business Chamber's Lunchtime Mixer
Texas Roadhouse – ear
Date: February 6, 2020
Time: 12:00 PM – 2:00 PM EST
Location: 250 Buckley Boulevard
Bear, DE
Estate Planning Seminar
Estate planning for young adults by Estate & Elder Law
Learn personal and business aspects of estate planning
Date: February 19, 2020
Time: 9:00 AM – 10:30 AM EST
Location: DSBC Office – 11F Liberty Plaza, Newark, DE 19711
All About YOU
A Unique Vendor Event
There will be vendors, speakers and prize drawing games with educational and informational 60 second tips throughout the day!
Date: February 28, 2020
Time: 10:00 AM – 2:00 PM EST
Location: DoubleTree Hotel – 4727 Concord Pike, Wilmington, DE
Business Owners ONLY - Best Practices Round Table
The most proven way to success is learning from the others that have success
If you can avoid the mistakes and get the best ideas, then your probability of success skyrockets overnight and you surround yourself with people that can help you succeed.
DATE:Jan 8th and then 1st Wednesday each month
LOCATION: DSBC Office 11F Liberty Plaza, Newark – Bring your own lunch (Microwave & Toaster Oven available if needed)
Membership Goal
Help us reach our 2020 goal of 400 Active Members.
Here is where we stand as of today:
- Percentage of our goal as of today. 75% 75%
The Inside Scoop
What sets us apart from other chambers
What sets the Delaware Small Business Chamber apart from all other. Watch this video. (Thanks Bruce Productions)
2018-2019 State of the Chamber Video
This is our annual State of the Chamber video giving the viewer a synopsis of what we accomplished last year and are planning for the upcoming year.
Things you may want to know about us.
Thanks to Bruce Productions for this video about a variety of benefits and items the the Delaware Small Business Chamber offers to members.
Local Author and DSBC Member Struck By Lightning
FOR IMMEDIATE RELEASE 352 Hackberry Drive New Castle, De 19720 302-229-3446 firstname.lastname@example.com www.gowithinspiritualcoaching.com Local author reveals inner struggles that led to devastating consequences of addiction, and how she overcame them. New...


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Teacher: Marie Takahashi (Berlin)
Speaks English, French, German
Einzelne/Gruppe Unterricht für Viola !
Alle Niveau, alle Alter, alle Genre sind willkommen!
Private / group lesson for Viola!
All levels, all ages, all genres are welcome!
Cours privé / en groupe de l'alto!
Tout les niveaux, âges, genres sont bienvenus!
I'd like to offer each lessons with three important parts...basics, solo-approach and ensemble!
To play with another people is a fantastic element of music.
Lessons in person or online:
Hourly rates: (EUR €)
1 student: €25.00
2 students: €20.00
3+ students: €15.00
Fees apply. View details.
We will find a tutor for you.
Berlin has about six million residents from over 180 different nations. Berlin is considered an important cultural, political and scientific node at the international level, in addition to having one of the highest standards of living in the world and being an important tourist destination.
German is the dominant language in Berlin, but about 30% of its inhabitants are of foreign origin. The most-commonly-spoken foreign languages in Berlin are Turkish, Russian, Arabic, Polish, Kurdish, Vietnamese, English, Serbian, Croatian and Greek, among others.

subset: commoncrawl


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*Airport transfers are included as part of the group. If you are unable to travel with the group, you'll need to make separate arrangements. You will be notified via email as soon as you book as to what times the airport coach will depart so that you may make your flight reservations accordingly. We understand that flights arrive and depart at different times and plan ahead for that. We do adjust travel plans to try and accommodate everyone however, if you are unable to travel with the group, please contact us, we're here to help!
**Rustic Tuscany tour includes all breakfasts, lunches and dinners: see itinerary for further detail on venue and timing
This website uses cookies to improve your experience while you navigate through the website. Out of these cookies, the cookies that are categorized as necessary are stored on your browser as they are as essential for the working of basic functionalities of the website. We also use third-party cookies that help us analyze and understand how you use this website. These cookies will be stored in your browser only with your consent. You also have the option to opt-out of these cookies. But opting out of some of these cookies may have an effect on your browsing experience.
Necessary cookies are absolutely essential for the website to function properly. This category only includes cookies that ensures basic functionalities and security features of the website. These cookies do not store any personal information.


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INRODUCING: Temple Songs
I was sent the track 'Passed Caring' this morning which is the debut single by Temple Songs, on first listen I got them mixed up with Temples, similar name and very similar sound (yeah im stupid). But these guys are definitely not Temples; they are a Manchester four-piece made up of Jolan Lewis (guitar vocals) Dave Hardy (bass) Jean Hughes (guitar) Andrew Richardson (drums) They have been doing the rounds over the past year supporting some of the best emerging talent including; Temples, Charlie Boyer And The Voyeurs, METZ, Egyptian Hip Hop and Palma Violets
Passed Caring is a lovely fuzzy little number and is a strong debut from the Manchester quartet, it's woozy, trippy, psychedelic and recorded with a lo-fi edge (they like to record onto cassette) and on Passed Caring you feel the 60's inspiration coming from the likes of The Beach Boys and the LSD influenced tracks off The Beatles Revolver album
Temple Songs will be playing Dalston's Shacklewell Arms on June 27th for the Passed Caring launch party.
Passed Caring will be released via RIP Records on July 1st 2013 (7" Vinyl)


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University of Southern Denmark
Designed by Danish Architects Henning Larsen, the University of Southern Denmark is a significant landmark in Kolding. The shape of the building and its facades create a powerful dialogue between the inner life of the building and the outside observer.
The facade is an integrated part of the building and creates a unique and varying appearance, with exposed large balconies made from Kebony Clear cladding and decking. Alongside eco-friendly Kebony wood, the building features a number of other sustainable initiatives, such as cooling by means of water from Kolding River, low-energy ventilation and solar cells.


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Cardinals Game 1 starter Adam Wainwright: World Series opportunity 'pretty special to me'
Cardinals Game 1 starter Adam Wainwright wasn't about to disclose any secrets about attacking the Red Sox lineup. "I can't tell you that, can I?" he chuckled. "That's the scouting report." He did, however, suggest that the opportunity to pitch in the World Series -- after being unable to do so in 2011, when he was sidelined while recovering from Tommy John surgery -- represented a special moment for him. He'd pitched in the World Series before, of course, having emerged as the closer on the 2006 Cardinals team that enjoyed a surprise march to a title, but to return to that platform after rehabbing in 2011 and enduring a return in 2012 in which his arm strength fluctuated represents a different sort of accomplishment. "It's pretty special to me," said Wainwright. "I never doubted that I would return, but those thoughts creep in. ... My stuff came back, my ability that I knew was there kind of returned. To be able to have some big-time playoff moments this year, it's been very special, something I'll never forget." One interesting aspect of facing the Red Sox that Wainwright did explore was facing Shane Victorino, who has set a record by getting hit six times in the postseason this year. "I've pitched against Shane many years. I know if he gets on base, he can wreak havoc. He's very fast. He's a very good baserunner. So I don't think anyone in our locker room is intentionally ever going to throw one and hit him on purpose because they know what they can do on the basepaths," said Wainwright. "I saw a couple of those [HBPs]. They were breaking balls and changeups, too. It's unintentional sometimes." Wainwright, who has faced Victorino 23 times, suggested that there would be a fascinating full-circle moment in the opportunity to face the outfielder -- a switch-hitter for most of his career -- batting right-handed, given that Wainwright's experience facing Victorino dates to the outfielder's first explorations of hitting left-handed. "It'll be interesting to see him right-handed. I faced him left-handed quite a bit, and I remember his first game attempting to switch-hit when he was with the Dodgers in Double-A," said Wainwright. "I played against him way back when. All he could do was slash and run. Next year, he came back and had great power from the left side, even more power, I think, lefty than righty. So it'll be interesting to see him hitting right-handed." Wainwright also expressed his amazement at Red Sox closer Koji Uehara's ability to strike out opponents, suggesting that his ability to elicit three-pitch punchouts was cartoonish. "We're going to do our best to not let him pitch at the end of the game," said Wainwright.


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Primary 1 were delighted to welcome Leon's Dad Henry to class today. He talked to us all about his career as an animator. We got to see some of the animations he has made and he explained some of the different jobs he gets to do.
We really loved it when he showed us how to make a simple stop-motion animation about a cat. It was very funny and has inspired us to have a go ourselves!


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The X Factor has undergone a huge makeover for the celebrity version of the show.
Judge Louis Walsh has revealed that two of the show's most-loved segments have been axed from The X Factor Celebrity.
In the new series viewers won't get to see with the boot camp stage or the incredibly tense six chair challenge.
The six chair challenge saw the judges whittle down which acts they were going to take through to judges' houses by offering them a 'chair' in their line up of finalists.
It's likely this part has been thrown out as there aren't enough contestants to make the six chair challenge enough of a battle.
Louis explained: 'What we're doing this year I think is a brilliant idea. I think everyone's going to love watching these celebrities because it's not what people expect.
'Some of them are really good. The show feels more exciting. There's no Bootcamp, no Six-Chair Challenge, it feels slick this year.
'It's been the best show on TV for a long time and has just had a little rebranding, I suppose, a new X Factor.'
The music manager joins Simon Cowell and Nicole Scherzinger on the judges' panel.
A new trailer for the show saw Simon, Nicole and Louis listening to the celebs do their thing in a luxury Hollywood venue, which we think is a fair replacement for judges' houses.
Reality star Megan McKenna, Glee's Kevin McHale, EastEnders' Jonny Labey will all be competing in the Unders category. The Overs is comprised of journalist Martin Bashir, actress Victoria Ekanoye and talk show host Ricki Lake.
In the groups will be a Love Island supergroup comprised of Wes Nelson, Samira Mighty, Eyal Booker and Zara McDermott. Ben Foden, Thom Evans and Levi Davis will be teaming up for a group, along with Brendan Cole and Jeremy Edwards.
Megan was recently spotted welcoming Louis to her home as the pair filmed scenes for the show.
Given how happy the pair looked it's safe to assume that the Towie star's time on the show is going well.
The X Factor Celebrity starts Saturday 12 October at 8.35pm.
Got a showbiz story?
If you've got a celebrity story, video or pictures get in touch with the Metro.co.uk entertainment team by emailing us email@example.com, calling 020 3615 2145 or by visiting our Submit Stuff page - we'd love to hear from you.
MORE: Downton Abbey bosses ask Julian Fellowes for sequel as movie rakes in £120 million
MORE: The Greatest Bake Off: Sandi Tokvig makes dig about Henry's 'girlfriend' amid Alice dating rumours


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This report provides you all of the information you will need to learn the best cosmetic product. There are two broad kinds of cosmetic skin care natural and chemical. As is evident from the title, the former technique uses chemicals and pharmaceutical chemicals. Now, while most of these chemical laden creams are ineffective, those that work they also bring a whole lot of unwanted effects along. So, chemical laden cosmetic skincare products aren't something that I prefer. With organic skin products already available on the current market, I don't really feel the need of exposing my skin to the harsh substances that instead of doing any good to it might harm it further. In contrast, natural skin products are completely safe to be used. They have the potential and strength of known organic herbs and substances which could provide you wondrous results.
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@Dreadshadow: Thanks! I'm glad you liked it~ and yeah my bad. I kind of rushed the submission so I must have forgotten. My ReStaff resources are all free for use both commercial and noncommercial and requires you to credit me when used. : ) I believe I also said RPGMaker games only. And optionally it'd be great to hear from people who use them~ just because I'm curious about where they go.


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Edwin Cartlidge
Armed with new kinds of atomic clocks, scientists are planning to overhaul the unit of time.
[Getty Images]
Physicists with the NIST-F2 cesium fountain clock in Boulder, which has served as a U.S. civilian time and frequency standard since 2014. [NIST]
In November 2018, representatives of 54 countries met in Versailles, France, to approve a major revision to the International System of Units (SI). Delegates at the General Conference on Weights and Measures (CGPM) agreed to redefine four of the seven base units—meaning that, for the first time in history, all units refer to constants of nature. Notably, the kilogram had until that point been defined by the mass of a platinum-iridium cylinder held in a basement on the outskirts of Paris.
On this occasion, the second was not in the spotlight, even though it remains the cornerstone of the SI system. It was redefined in 1967 as "the duration of 9,192,631,770 periods of the radiation corresponding to the transition between the two hyperfine levels of the ground state of the cesium 133 atom." Bar a little rewording, that definition remains in place today. But behind the scenes, metrologists are busy planning a makeover. The idea is to replace the microwave definition with one based on a far higher optical frequency.
The overhaul could lead to new and improved applications of precise timekeeping, such as better navigation of spacecraft and more sensitive searches for any variations in the fundamental physical constants. The push comes from rapid advances in technology, with the best optical clocks now significantly outperforming the cesium devices that serve as the standards for international time.
Last year (February 2018), a committee of metrologists from the International Committee for Weights and Measures (CIPM) published a "roadmap" laying out a series of milestones that the committee says need to be passed in order to redefine the second. Since then, two groups claim to have taken the important first step along that road—demonstrating optical clocks that would be at least 100 times as accurate as the world's best cesium timepieces, were the second to be defined in terms of visible light.
Fritz Riehle of Germany's PTB national metrology institute in Braunschweig, and one of the roadmap's authors, says that industry and most other users "will sleep well enough" with the microwave definition in place for the time being. But he reckons that it makes sense to redefine within the next decade, in part to save money that would be used to make cesium clocks more accurate. "We would spend a lot of time making inferior clock technology better," he says.
Indeed, according to Tetsuya Ido of Japan's National Institute of Information and Communications Technology, scientists' enthusiasm for optical clocks is hampering the maintenance of the most accurate microwave devices, known as cesium fountains. In fact, he believes that within a couple of years the PTB and its French equivalent SYRTE in Paris might be the only labs in the world operating stable fountain clocks, saying, "We may have to rush to make a new definition."
[Illustration by Phil Saunders] [Enlarge image]
All clocks rely on some kind of regular, periodic "tick" to keep track of passing time. A clock's accuracy—how close its measured second is to the "real" value—usually depends on the kind of tick employed and how well the device is built. Ultimately, however, it is limited by how the second itself is defined. In the past, that quantity was stipulated to be 1/86,400 of the length of a day. But because the Earth's rotation on its axis varies very slightly, so did the length of a second—by around one part in 107. The definition was then reformulated in terms of Earth's rotation around the Sun, which made it more accurate but quite unwieldy.
Then came atomic time, and the accuracy of the second subsequently shot up by many orders of magnitude. This fact is exploited today in many technologies that rely on precision timekeeping, including cellphone networks, electricity grids, satellite navigation and more. But, even here, the second's definition imposes a cap on accuracy.
Cesium fountains use lasers to cool a gas of cesium atoms and then launch them upwards through a tube—like droplets of water in a fountain. As the atoms rise and then fall back to Earth, they pass through a field of microwaves, often generated by a crystal oscillator, which excites some of them and creates fluorescence (after stimulation by a suitable laser). By varying the microwave frequency slightly from one launch to the next and monitoring the resulting change in fluorescence, the device is able to lock the oscillator frequency to the hyperfine transition—since at this point the output peaks.
A strontium lattice clock at the PTB metrology lab in Braunschweig, Germany. [Physikalisch-Technische Bundesanstalt]
Any atomic clock probes its timekeeping atoms by scanning the radiation from an oscillator across a fairly narrow range of frequencies and measuring the atoms' response. Accurately locating the peak in that output involves slightly de-tuning the oscillator until the output drops to 50 percent—a spread in frequency known as the linewidth.
Maximizing a clock's precision means reducing the linewidth as far as possible, but there is a fundamental limit imposed by quantum noise. In other words, there is a finite chance that any given atom won't be excited. This random noise can be averaged away by interrogating multiple copies of the same atom and by repeating the measurement many times. However, this takes a while in microwave clocks due to their much lower frequency.
Because each measurement lasts about a second in both cesium fountains and optical clocks—set by the time of atoms' free fall and the coherence time of the probing laser, respectively—the linewidth is about 1 Hz. Since noise decreases as the square root of both the number of atoms and number of measurements, a cesium clock with a transition frequency of 1 gigahertz that contains a million atoms will yield a peak with a precision of one part in 1013 after a single measurement. Reaching a precision of 10−16 means nonstop measurements for 1 million seconds—at least a week.
In contrast, probing just 10,000 atoms using radiation at 1015 Hz yields a quantum-limited precision of 10−17 for a single measurement. This would average down to 10−18 in a couple of minutes. However, according to Jérôme Lodewyck at SYRTE, France, other sources of noise, particularly fluctuations in the laser frequency, mean that the precision of a single measurement is actually about 10−16. Still, he says, it is possible to achieve 10−18 after just "a few hours of measurement."
The best cesium fountains today have an accuracy—in other words, how close their frequency is to the true, unperturbed value of the hyperfine transition—of 1.6 parts in 1016. This means, were longevity not an issue, they would neither lose nor gain more than a second in about 200 million years. That uncertainty can, in principle, be further reduced by eliminating all of the systematic effects that very slightly shift the frequency, such as stray electromagnetic fields. However, the fact that microwaves have a relatively low frequency makes any real improvement an uphill battle.
That's because frequency determines statistical precision. All else being equal, the time needed to reduce instability—the internal variation in ticking rate—below a certain level gets longer as the transition frequency goes down. (See "In search of stability," p. 46.) To reach 10−16, cesium clocks must run for about a week, so tweaking a clock to make it more accurate can involve months or years of work, making uncertainties below 10−16 an impractical goal, according to Jérôme Lodewyck, a metrologist at SYRTE, part of the Paris Observatory.
Optical clocks, with their much higher frequencies, in principle can be far more accurate. But the first such devices only started operating in 2001, once physicists had overcome a number of technical hurdles, such as developing lasers with very stable frequencies. Also key was the invention of the frequency comb, which compares the frequency of two electromagnetic waves—yielding an absolute value (in hertz) for an optical clock's output when referenced to a cesium timekeeper and a simple ratio when measured against another optical device.
Despite the late start, optical clocks quickly outperformed their microwave counterparts. While seconds remain defined in terms of cesium, no optical clock can be more accurate than the best cesium clock by definition, so scientists instead talk in terms of "systematic uncertainty." And by 2008, optical clocks had achieved lower uncertainties than the best microwave devices—some 10−15.
This rapid progress led the CIPM to set up a list of "secondary representations of the second"—a number of mainly optical transitions whose frequencies and uncertainties are monitored against those of cesium so that optical clocks can also be used to keep time. When one of these (or perhaps a transition still to be exploited) then becomes the frequency used to define the second, cesium-133 will be relegated to secondary status. It was to ensure that this transition is as smooth as possible that the CIPM published its roadmap in February 2018.
The first milestone on the roadmap now appears close to completion. It states that at least three different optical clocks, either in different labs or of different types, must exceed the systematic uncertainty of the best cesium clocks by "about two orders of magnitude." Two groups claim to have achieved that, through quite different approaches.
Andrew Ludlow and colleagues at the National Institute of Standards and Technology (NIST) in Boulder, Colo., USA, reported in July 2018 that they had reached an uncertainty of 1.4×10−18 using what is known as an optical lattice clock. First demonstrated by Hidetoshi Katori and colleagues at Tokyo University, Japan, this involves using tightly-focused lasers to cool and trap thousands of neutral atoms in a lattice of standing waves before using a "clock laser" (pre-tuned inside an optical cavity) to excite the atoms. Ludlow's team has done so using ytterbium atoms.
The electrode system of the trap used to store an ytterbium ion in an optical clock at the PTB metrology lab in Braunschweig, Germany. [Physikalisch-Technische Bundesanstalt]
That work has now been ever so slightly bettered by a rival group, also at NIST, which uses the other main type of optical technology—trapped ions. David Leibrandt and colleagues trap a single ion of aluminum in an oscillating electric field and cool it via Coulomb interaction with a magnesium ion. Over the past five years, the group has reduced the already tiny Doppler shift of the aluminum ion's frequency by better controlling the trapping field. In a paper targeted for submission in January 2019, the team reports a systematic uncertainty of 9×10−19.
Meanwhile, Jun Ye and colleagues at the JILA research institute, just a couple of kilometers down the road in Boulder, have achieved 2×10−18 with a strontium lattice clock, while Ekkehard Peik and co-workers at PTB in Germany have reached 3×10−18 using an ytterbium ion.
However, while individual groups reach and even go beyond the CIPM's uncertainty threshold, more will have to be done before the second can be redefined. Both Ludlow's group at NIST and Peik's at PTB have made two versions of their respective clocks and compared their output to make sure they keep time to within their combined uncertainties. However, as Lodewyck points out, stray fields or other systematic shifts could conceivably throw off two clocks within a given lab by the same amount. "Only when you compare clocks built by different teams," he says, "can you prove that clocks are correct."
While individual groups reach and even go beyond the CIPM's uncertainty threshold, more will have to be done before the second can be redefined.
While individual groups reach and even go beyond the CIPM's uncertainty threshold, more will have to be done before the second can be redefined.
One way of doing this is to measure the ratio of frequencies from two different types of optical clock and then compare that to the same ratio measured in another lab. Alternatively, two clocks of the same type can be compared across labs, either by using portable clocks as a go-between or by hooking the clocks up to one another via fiber optic cable.
In Europe, scientists have set up new fiber links between the PTB and SYRTE (and, more recently, the NPL). To avoid the excessive attenuation of visible light, researchers at both ends of the link split the beam from a 1.5-micron (infrared) laser and then use a frequency comb to compare the wavelength from one half of that beam with the output of their optical clock while sending the other half down the fiber. The two halves of the different 1.5-micron beams then meet in the middle (Strasbourg, France), where their frequencies are compared.
The latest measurements were carried out last June. Lodewyck says that although most of the (six) clocks being tested agreed with one another to better than "a few parts in 1017," there were typically a couple that disagreed by more than the uncertainties attributed to them. For instance, he says, the frequency of a strontium lattice clock at SYRTE shifted because residual air molecules interacted with atoms in the system. "We had underestimated this systematic effect before," he says.
It is for exactly this reason that metrologists tread carefully when it comes to published uncertainties. A CIPM working group on frequency standards meets periodically to generate best estimates for the values and systematic uncertainties of the various secondary representations of the second and, to be on the safe side, often boosts the combined uncertainties by a factor of two or three.
The nightmare scenario is a step change in the value of the second. This would occur if, after a redefinition, it turned out that the claimed uncertainty for the optical transition in question was too low—so much so that the measured frequency of the cesium-133 transition then becomes very slightly more or less than its (previously defined) whole number of hertz, when considering up to six decimal places. "You can find yourself in trouble if you are not careful," says Patrick Gill of the National Physical Laboratory in the U.K., who until last year was working group co-chair (with Riehle).
[Adapted from Meynadier/Le Targat/Pottie/LNE-Syrte / Inset schematics by Phil Saunders] [Enlarge image]
To ensure that there is, in fact, a smooth transition between microwave and optical definitions, the CIPM roadmap also stipulates that the frequency of the chosen optical technology has to be compared against that of the best cesium fountains. If the optical clocks work as claimed, then the accuracy of such measurements would be entirely limited by the fountain clocks.
But there is one more thing that metrologists want to see before they unleash a revamped second: optical clocks contributing regularly to global timekeeping. National labs currently generate the real-time signals for (approximate) Coordinated Universal Time (UTC) using hydrogen masers and commercial cesium clocks that are, in some cases, corrected periodically by cesium fountains and are compared via satellite links. Official UTC is in fact a "paper" timescale that the CIPM's secretariat works out once a month by taking a weighted average from hundreds of clocks at participating labs. Scientists hope that over the next few years several optical clocks will start to contribute to UTC. (Until recently, only a strontium lattice device at SYRTE had done so.)
In Japan, Ido and colleagues have shown they can deliver an ongoing timescale by using a strontium lattice clock to stabilize and calibrate a continuously running hydrogen maser (masers being very reliable and stable for a few hours but tending to drift over longer periods). By running the optical clock for just three hours a week, they were able to generate a signal that deviated from UTC by just 0.8 nanoseconds over the course of six months—a fractional difference of only 5×10−17.
Ido hopes that within a few years one of the three masers used by his institute to generate Japan Standard Time can be "steered" by an optical clock instead of an ensemble of cesium clocks. But the longer-term goal, he says, is all-optical timekeeping, in which strontium lattice clocks, for example, run continuously—replacing both masers and cesium devices.
However, Lodewyck says that optical clocks' complexity means that they are likely to run intermittently for some time yet, and that masers may remain the workhorses of UTC even after the second is redefined. He points out that the roadmap does not require ditching masers altogether, and that future timekeeping is likely to be limited by the satellite links between national metrology labs, which are good enough to compare microwave signals but not optical ones. Extending fiber links across oceans, on the other hand, will be technically demanding and expensive, he says.
One fundamental issue that needs to be resolved is choosing the type of atom—and hence type of clock—that will come to define the second.
One fundamental issue that needs to be resolved is choosing the type of atom—and hence type of clock—that will come to define the second.
Another, more fundamental, problem comes from general relativity: the different ticking rates across the Earth's surface due to variations in height and hence gravitational field. In fact, a difference in elevation of just 1 cm changes ticking by 10−18. A possible solution is to put one or more master clocks in space, but that would require major leaps in satellite technology and so likely remains a long-term ambition, says Lodewyck.
In truth, scientists disagree about how urgent the need for a redefinition is. Riehle argues that an early change would give scientists and engineers a chance to develop new applications. Conversely, his PTB colleague Peik reckons that in the absence of demanding new applications, the existing cesium infrastructure is perfectly adequate. Nevertheless, all agree that the next CGPM, due in 2022, will be too early, making the one after that—in 2026—the first realistic opportunity to approve the overhaul.
One fundamental issue that needs to be resolved is choosing the type of atom—and hence type of clock—that will come to define the second. The strong suit of atomic lattices is stability, given the large number of atoms—each in effect a time keeper—that are involved. According to Gill, lattice clocks are typically about 10 times as stable (after a given running period) as ion clocks.
Laser beams are used to create an atomic clock involving a tiny three-dimensional cube of strontium atoms. [G.E. Marti/JILA]
Indeed, Ye and colleagues at JILA have made a clock from a quantum gas of strontium atoms trapped in a 3-D optical lattice that can reach a precision of 3×10−19 after only about two hours of operation—thanks to a high density of atoms within the trap. That, in turn, makes him optimistic that they can lower systematic uncertainties as well. But he admits that there are a couple of frequency shifts that could prove difficult—those due to the trapping light and blackbody interference.
Leibrandt reckons that the cleaner environment of a single ion—largely free from interactions with other particles—could prove decisive in the push for accuracy. He says it might be possible to further reduce the systematic uncertainty of aluminum ions by a factor of 10 over the next five years. Meanwhile, Tanja Mehlstäubler and others at PTB are developing symmetrical traps that they say could allow several tens, if not hundreds, of ions to be probed with systematic uncertainties as low as 10−19, raising the prospect of very stable ion clocks.
Gill maintains that it might still take several years for a winner to emerge between lattice and ion clocks (although he says that their superior stability might eventually give lattice clocks the edge). He points out that as well as being accurate and stable, optical clocks must also be easy to use are if they are to become widespread. Nevertheless, he reckons, if the uncertainties of rival clocks differ by no more than a factor of 10, then choosing between them will be tough. "The community has to come to a consensus," he says. "There will be a lot of to-ing and fro-ing."
Edwin Cartlidge is a freelance science journalist based in Rome.
F. Riehle et al. "The CIPM list of recommended frequency standard values: Guidelines and procedures," Metrologia 55, 188 (2018).
W.F. McGrew et al. "Atomic clock performance beyond the geodetic limit," https://arxiv.org/abs/1807.11282 (2018).
C. Lisdat et al. "A clock network for geodesy and fundamental science," Nat. Commun. 7, 12443 (2016).
H. Hachisu et al. "Months-long real-time generation of a time scale based on an optical clock," Sci. Rep. 8, 4243 (2018).
S.L. Campbell et al. "A Fermi-degenerate three-dimensional optical lattice clock," Science 358, 90 (2017).
J. Keller et al. "Probing time dilation in Coulomb crystals in a high-precision ion trap," https://arxiv.org/abs/1712.02335 (2018).
Publish Date: 01 February 2019
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Kruger National Park primarily caters to nature and animal lovers. At natural landmarks like the Kruger Tablets and Hippo Pool, visitors will likely see lions lounging and hippos swimming. Meanwhile, game drives and bush walks allow travelers to spot must-see animals like Nile crocodiles, elephants, giraffes and rhinos. More traditional vacation pursuits like guided mountain bike excursions and golfing are also available here. And for those who enjoy archaeology and history, do not pass up a chance to explore the Albasini Ruins.
Updated March 28, 2019
- #1View all Photos#1 in Kruger National ParkHiking, Recreation, Sightseeing, ToursTYPE2 hours to Half DayTIME TO SPENDHiking, Recreation, Sightseeing, ToursTYPE2 hours to Half DayTIME TO SPENDRead More
If you don't have multiple days to spend at in-park trails like Wolhuter and Nyalaland but want to explore the area on foot, consider signing up for a river walk or a morning or afternoon bush walk. These two- to four-hour walks depart daily from main rest camps like Letaba, Lower Sabie, Olifants, Satara and Skukuza. However, river walks by the Olifants River are only offered at the Olifants rest camp. Each walk is led by two experienced guides.
Large game, birds and insects are regularly spotted during bush walks, so bring your camera with you. Do not be startled to see your guides carrying loaded rifles; rangers are armed solely to protect you from animals. And as an added precaution, you will be asked to wear neutral colors, which help you blend in with your surroundings. Recent travelers recommend the bush walks offered at Lower Sabie and Satara.
- #2View all Photos#2 in Kruger National ParkMonuments and Memorials, Natural Wonders, Sightseeing, FreeTYPELess than 1 hourTIME TO SPENDMonuments and Memorials, Natural Wonders, Sightseeing, FreeTYPELess than 1 hourTIME TO SPENDRead More
Though Kruger boasts several locations where lions are known to linger, one of the best places to spot the park's big cats is atop the Kruger Tablets. Nestled along the southern edge of Nkayeni Region, the Kruger Tablets are dedicated to Paul Kruger, the founder of the Sabie Game Reserve, which later became Kruger National Park. A plaque on one of the site's rocks can still be seen from the adjacent road.
Lions enjoy lounging on rock formations, so it's hardly surprising that Kruger's rock pilings – including the Kruger Tablets – are a popular lion haven. Odds are you'll snap tons of photos of these animals while in the area. But remember: Lions are dangerous animals, so stay in your car or safari vehicle at all times.
- #3View all Photos#3 in Kruger National ParkSightseeing, ToursTYPE2 hours to Half DayTIME TO SPENDSightseeing, ToursTYPE2 hours to Half DayTIME TO SPENDRead More
An easy way to search for animals in Kruger National Park is to sign up for a game drive. Departing from all bushveld and main rest camps throughout the day and night, the park's game drives offer visitors a chance to see wildlife from the comfort of an open-air vehicle while enjoying commentary from an experienced guide. Animals commonly spotted on game drives include elephants, giraffes, lions and impala.
Game drives are available at sunrise, sunset and night. Each time of day and camp provides travelers with different game-viewing opportunities, so consider booking multiple drives while in the park. Additionally, drives last two to three-and-a-half hours, so dress and pack accordingly. Long-sleeved clothes and a jacket, sunscreen and water are highly recommended. Travelers can also bring snacks, but remember to keep items secure at all times and to dispose of garbage in designated trash bins.
- #4View all Photos#4 in Kruger National ParkNatural Wonders, Sightseeing, FreeTYPELess than 1 hourTIME TO SPENDNatural Wonders, Sightseeing, FreeTYPELess than 1 hourTIME TO SPENDRead More
As its name implies, Hippo Pool – which sits near Kruger's southern border – acts as one of the park's premier locales for viewing hippos. In fact, hundreds of these giant, grunting creatures frequent this part of the Crocodile River, where they spend the majority of their time soaking in the water to stay cool. Crocodiles also reside here but are typically harder to spot.
Visitors are more than welcome to get out of their vehicles at Hippo Pool. However, hippos are extremely dangerous, so stay in designated viewing areas at all times. For the best hippo photos, arrive around dusk when these creatures climb ashore to eat grass.
- #5View all Photos#5 in Kruger National ParkNatural Wonders, Sightseeing, FreeTYPELess than 1 hourTIME TO SPENDNatural Wonders, Sightseeing, FreeTYPELess than 1 hourTIME TO SPENDRead More
Situated near the Shingwedzi River in the park's Nxanatseni Region, the Red Rocks are beautiful to admire. Exposed after years of wear by the adjacent river, the Red Rocks offer a stark contrast to Kruger's trees and savanna grasslands. Plus, these sandstone slabs are regularly visited by must-see animals like elephants, giraffes and lions.
If you want to check out the Red Rocks, consider staying at Shingwedzi rest camp, which is located less than 15 miles away. The sight can be accessed by car or safari vehicle, though game drive routes vary depending on the guide. Driving can be a bit tricky in this part of the park, so ask for detailed directions from a Kruger employee before heading out.
- #6View all Photos#6 in Kruger National ParkHiking, Recreation, SightseeingTYPEMore than Full DayTIME TO SPENDHiking, Recreation, SightseeingTYPEMore than Full DayTIME TO SPENDRead More
Located in Kruger's Marula Region, Wolhuter Trail features one of the park's more unique landscapes and some of the best opportunities to spot wildlife. The area's granite outcrops and deep valleys are regularly frequented by animals like elephants, zebras, giraffes and black and white rhinos. An array of birds are also seen here often. What's more, visitors can catch a glimpse of historic relics that date back to the Stone and Iron ages on many of the trail's rock formations.
According to recent travelers, Wolhuter Trail offered some of the best game-viewing and bush accommodations in the park. Plus, many loved the catered meals provided and described the rangers as "friendly" and "knowledgeable." But keep in mind that this area requires a three-night stay, so plan accordingly. Visitors with limited time may want to consider skipping Wolhuter Trail in favor of a bush walk from a traditional rest camp. Also, age and fitness restrictions apply, so consult Kruger National Park's website before booking a stay here.
- #7View all Photos#7 in Kruger National ParkSightseeing, FreeTYPELess than 1 hourTIME TO SPENDSightseeing, FreeTYPELess than 1 hourTIME TO SPENDRead More
One of two sites with ruins found inside Kruger's gates, the Albasini Ruins offer a look into the park's rich history. This locale houses the remains of a 19th-century trading post, where goods like beads, clothes and metal products were once traded between Portuguese colonists and the indigenous Ba-Phalaborwa. All that remains today are a few crumbled walls and some artifacts, but history buffs will likely enjoy snapping some photos and perusing the attraction's display cases.
Travelers who are not fond of history may want to skip the Albasini Ruins. But for those who pass through Phabeni gate, which is less than a half-mile away from the attraction, stopping here may be worthwhile. The Albasini Ruins also offer a change of scenery from the park's animal-focused activities.
Explore More of Kruger National Park
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There are more iPhones sold each day than babies born in the world.
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Personal devices increase productivity, but can quickly become a liability without proper endpoint security. Your CIO's top priority may be security, but your end users value productivity above all else. We don't think IT professionals should have to choose between these often-competing goals. We let them say "yes" to both.
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During the Age of Enlightenment, as Sir Isaac Newton was watching apples fall, another brilliant physicist, Emilie du Châtelet finds herself with child. At 42, fearing she will die in childbirth, she races to complete her research and leave her legacy. Meanwhile, present day scientist Olivia, unable to conceive and wondering what she will sacrifice for motherhood, arranges for a surrogate, who pulls together past and present in a stellar collision.
By Karen Zacarias
Directed by Lois Roach
Lyric Stage Company of Boston
Feb 12 – Mar 13, 2010
Sarah Newhouse, Diego Arciniegas, Jonathan Popp, Susanne Nitter, and Rosalie Norris, Allan Mayo, Jr
Design Team:
Janie E. Howland, Scenic Design
Charles Schoonmaker, Costume Design
Scott Clyve, Lighting Design
Arshan Gailus, Sound Design
Photos courtesy of Lyric Stage Company of Boston (website | profile | tag archive).
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SCY2151 - The body, health and society
6 points, SCA Band 1, 0.125 EFTSL
Undergraduate Faculty of Arts
Leader(s): Alan Petersen
Clayton Second semester 2009 (Day)
This unit focuses on sociological theorising about the body and contemporary issues in health sociology. It covers the big human issues of birth, sex, reproduction and death and the important social divisions of class, gender, ethnicity and sexuality. We will discuss embodiment and change, how health inequalities are socially produced and distributed and power relations in the current health care system.
By the completion of the unit the student should be able to:
- articulate a sound understanding of the sociological imagination or perspective;
- analyse complex health issues using a sociological perspective;
- articulate how our bodies are socially constructed;
- discuss the operation of medical dominance within the health system;
- demonstrate skills in synthesizing information and presenting an argument within class and in a report format.
Written work: 50% (2500 words)
Class test: 40% (2 hours)
Participation: 10%
Contact hours
1 one hour lecture and 1 one-hour tutorial per week
A first-year sequence in Sociology or permission
13 October 2017 20 January 2020


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David Carrier
Deputy Director, Communications
David Carrier serves as Deputy Director of Communications. He has designed and implemented communications strategies for nonprofit organizations for 20 years.
Prior to joining Council for a Strong America in 2011, David was the Director of Outreach and New Media at Child Trends, where he shared the latest research on children and families with media, policymakers, and practitioners, and also pioneered the organization's use of social media.
David has also managed projects and conducted outreach for the National Collaboration for Youth, American Planning Association, and National 4-H Council. David has a J.D. from American University and a B.A. from Brandeis University.


text:
Next Wednesday, 16th December 2015, at 5.00 pm, in our headquarters located in Piazza San Firenze 3, the President Maurizio Sangalli and our scholarship owners will illustrate the achieved outcomes and the researches in progress, one year on from the inauguration of our Institute. In honour of the occasion, the chief-rabbi of Florence Joseph Levi; don Luca Mazzinghi, professor at the Facoltà teologica dell'Italia centrale and President of Italian Biblical Association; and imam Izzeddin Elzir, President of UCOII, will be with us to present the initiative 'Religion is served. Jews, Chistians and Muslims come together … eating', expected for the first months of 2016. A tasting menu of Jewish, Christian and Muslim typical dishes, cooked by the students of the catering Institute 'Aurelio Saffi' of Florence, will follow. Download here the programme for further information.
Here is the programme of the Global Mayors Conference 'Unity in Diversity', that will take place in Palazzo Vecchio in Florence from next November 5th to 8th. The Sangalli Institute will participate to the conference with the appointment of a new scholarship: in fact, the last day the Mayor of Florence Dario Nardella will award, on behalf of the Institute, dr. Aitana Guia for the research plan 'Cities and the peaceful coexistence of the faiths: best practices, past and present'. Download the programme for more details.
After the summer break, we restart with the launches of new books: next Tuesday 13th October 2015, a new appointment with the Nicoletta Marcelli's essay on the teacher of Lorenzo il Magnifico, 'Gentile Becchi. Il poeta, il vescovo, l'uomo', Le Lettere editore, a fascinating tableau about Florence during the second half of the XVth century: see the programme in detail.
'Secularism and Religion in Modern Europe (XVIth-XVIIIth centuries)'. Workshop for young researchers
Here is the programme of the workshop for young researchers that our Institute will organize in Rome next 5th to 8th October 2015, in collaboration with the Escuela Española de Historia y Archeología, via di S. Eufemia 13. It is a new step in order to improve our international collaborations, focusing on some crucial aspects of the 'building' of Europe during the last centuries, and financially supporting young scholars. The workshop is organized by our vice-president Massimo Carlo Giannini and by Rafael Valladares as far as the Escuela. Renowned Italian and foreign scholars will be gathered in Rome together with a group of young researchers coming from European and non-European countries. Download the programme for more details.
In conjunction with the 'Maggio dei Libri 2015', the Sangalli Institute will organize, on Thursday 28th May, the second appointment of the month, that is the launch of Francesco Dei's book 'La Chiesa senza leggi. Religione e potere secondo un vescovo della Rivoluzione francese (1791-1794)', Morcelliana: see the programme in detail.
In conjunction with the 'Maggio dei libri 2015', the Sangalli Institute, in collaboration with Casa Buonarroti and the Opera Medicea Laurenziana in Florence and the University for foreigners of Siena, will organize on Thursday 14th May the launch of Andrea Felici's book 'Michelangelo a San Lorenzo (1515-1534). Il linguaggio architettonico del Cinquecento fiorentino', Leo S. Olschki: see the programme in detail.
The Sangalli Institute, in collaboration with the University of Valencia, has supported the international conference "¿Identidades religiosas en conflicto? Coexistencias, Intercambios y Enfrentamientos en el Mediterráneo (ss. XII-XVIII") / "Religious Identities in Conflict? Coexistence, Exchanges and Confrontations in the Mediterranean (12th-18th c.)", Valencia 7th-8th May 2015: see the programme in detail.
Paper and painted miracles: texts and images of the prodigious in Italy between XIVth and XVIIIth centuries
Interdisciplinary conference
Florence, 9th April 2015
Codes, structures and practices of the research on Middle Ages from the Unification of Italy to the First World War.
Sources and recent studies
Florence, 23rd-24th January 2015
Welcome address by the President of the Republic Giorgio Napolitano for the inauguration of the Institute