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: http://star.arm.ac.uk/~jgd/atomic_phy.html
Дата изменения: Tue Sep 18 17:11:04 2007 Дата индексирования: Mon Oct 1 23:33:14 2012 Кодировка: Поисковые слова: mercury surface |
However probably the most successful application of the atomic data have been to the development of electron density and temperature diagnostic emission line ratios for astrophysical plasmas, including the solar transition region/corona and late-type stellar atmospheres. Many diagnostics have been calculated over the past few years and applied to solar UV, EUV and X-ray solar spectra (obtained with the Solar Maximum Mission and P78-1 satellites, the S082A,B and S-055 instruments on board SKYLAB and the High Resolution Telescope and Spectrograph) on board SPACELAB 2), as well as UV observations of late-type stars obtained by the International Ultraviolet Explorer and Extreme Ultraviolet Explorer satellites. Several of these will be used by my students in their solar work involving data from the The CDS and SUMER onboard the SOHO and EIS onboard Hinode.