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BID : 1086_KF5JRV
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Subj: Atomic Time Standards
Path: IW8PGT<IZ3LSV<F1OYP<F4DUR<CX2SA<GB7CIP<N0KFQ<KF5JRV
Sent: 160406/1120Z 1086@KF5JRV.#NWAR.AR.USA.NA BPQ1.4.65

The "Atomic Age" of Time Standards

Scientists had long realized that atoms (and molecules) have resonances; 
each chemical element and compound absorbs and emits electromagnetic 
radiation at its own characteristic frequencies. 

These resonances are inherently stable over time and space. An atom of 
hydrogen or cesium here today is (so far as we know) exactly like one a 
million years ago or in another galaxy. Thus atoms constitute a 
potential "pendulum" with a reproducible rate that can form the basis 
for more accurate
clocks.

The development of radar and extremely high frequency radio 
communications in the 1930s and 1940s made possible the generation of 
the kind of electromagnetic waves (microwaves) needed to interact with 
atoms. Research aimed at developing an atomic clock focused first on 
microwave resonances in the ammonia molecule. In 1949, NIST built the 
first atomic clock, which was based on ammonia. However, its 
performance wasn't much better than the existing standards, and 
attention shifted almost immediately to more promising atomic-beam 
devices based on cesium.

Laboratory cesium frequency standard The first practical cesium atomic 
frequency standard was built at the National Physical Laboratory in 
England in 1955, and in collaboration with the U.S. Naval Observatory 
(USNO), the frequency of the cesium reference was established or measured 
relative to astronomical time. While NIST was the first to start working 
on a cesium standard, it wasn't until several years later that NIST 
completed its first cesium atomic beam device, and soon after a second 
NIST unit was built for comparison testing. By 1960, cesium standards 
had been refined enough to be incorporated into the official 
timekeeping system of NIST. Standards of this sort were also developed 
at a number of other national standards laboratories, leading to wide 
acceptance of this new timekeeping technology.

The cesium atom's natural frequency was formally recognized as the new 
international unit of time in 1967: the second was defined as exactly 
9,192,631,770 oscillations or cycles of the cesium atom's resonant 
frequency, replacing the old second that was defined in terms of the 
Earth's motions. The second quickly became the physical quantity most 
accurately measured by scientists. As of January, 2002, NIST's latest 
primary cesium standard was capable of keeping time to about 30 
billionths of a second per year. Called NIST-F1, it is the 8th of a 
series of cesium clocks built by NIST and NIST's first to operate on 
the "fountain" principle.

Other kinds of atomic clocks have also been developed for various 
applications; those based on hydrogen offer exceptional stability, 
for example, and those based on microwave absorption in rubidium 
vapor are more compact, lower in cost, and require less power.

Much of modern life has come to depend on precise time. The day is 
long past when we could get by with a timepiece accurate to the 
nearest quarter-hour. Transportation, communication, financial 
transactions, manufacturing, electric power and many other 
technologies have become dependent on accurate clocks. Scientific 
research and the demands of modern technology continue to drive 
the search for ever more accurate clocks. The next generation 
of time standards is presently under development at NIST, USNO, 
in France, in Germany, and other laboratories around the world.



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