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  2. Journal of Synchrotron Radiation - Wikipedia

    en.wikipedia.org/wiki/Journal_of_Synchrotron...

    The Journal of Synchrotron Radiation is a bimonthly peer-reviewed scientific journal published by Wiley-Blackwell on behalf of the International Union of Crystallography.It was established in 1994 and covers research on synchrotron radiation and X-ray free-electron lasers and their applications.

  3. Synchrotron radiation - Wikipedia

    en.wikipedia.org/wiki/Synchrotron_radiation

    Synchrotron radiation was first observed by technician Floyd Haber, on April 24, 1947, at the 70 MeV electron synchrotron of the General Electric research laboratory in Schenectady, New York. [5] While this was not the first synchrotron built, it was the first with a transparent vacuum tube, allowing the radiation to be directly observed.

  4. Synchrotron light source - Wikipedia

    en.wikipedia.org/wiki/Synchrotron_light_source

    Especially when artificially produced, synchrotron radiation is notable for its: High brilliance, many orders of magnitude more than with X-rays produced in conventional X-ray tubes: 3rd-generation sources typically have a brilliance larger than 10 18 photons·s −1 ·mm −2 ·mrad −2 /(0.1%BW), where 0.1%BW denotes a bandwidth 10 −3 ω centered around the frequency ω.

  5. National Synchrotron Light Source - Wikipedia

    en.wikipedia.org/wiki/National_Synchrotron_Light...

    The National Synchrotron Light Source (NSLS) at Brookhaven National Laboratory (BNL) in Upton, New York was a national user research facility funded by the U.S. Department of Energy (DOE). Built from 1978 through 1984, and officially shut down on September 30, 2014, [2] the NSLS was considered a second-generation synchrotron. [3]

  6. Sokolov–Ternov effect - Wikipedia

    en.wikipedia.org/wiki/Sokolov–Ternov_effect

    The Sokolov–Ternov effect is the effect of self-polarization of relativistic electrons or positrons moving at high energy in a magnetic field.The self-polarization occurs through the emission of spin-flip synchrotron radiation.

  7. Synchrotron function - Wikipedia

    en.wikipedia.org/wiki/Synchrotron_function

    In astrophysics, x is usually a ratio of frequencies, that is, the frequency over a critical frequency (critical frequency is the frequency at which most synchrotron radiation is radiated). This is needed when calculating the spectra for different types of synchrotron emission.

  8. Swiss Light Source - Wikipedia

    en.wikipedia.org/wiki/Swiss_Light_Source

    The Swiss Light Source (SLS) is a synchrotron located at the Paul Scherrer Institute (PSI) in Switzerland for producing electromagnetic radiation of high brightness. Planning started in 1991, the project was approved in 1997, and first light from the storage ring was seen at December 15, 2000.

  9. Synchrotron radiation circular dichroism spectroscopy

    en.wikipedia.org/wiki/Synchrotron_Radiation...

    Synchrotron radiation (SR) had been proposed for use as the light source at a meeting in Brookhaven National Laboratory on Long Island in 1972, [2] [3] however, it took a few years more before this came to fruition. Two research papers in 1980 reported the collection of CD data using SR as the light source for the experiments.