IDENTIFICATION OF EMISSION LINES IN A METEOR SPECTRUM OBTAINED ON AUGUST 2, 2011
نویسندگان
چکیده
منابع مشابه
emission lines in a high resolution extreme ultraviolet active region spectrum obtained by SERTS
New calculations of radiative rates and electron impact excitation cross sections for Fe XI are used to derive emission line intensity ratios involving 3s3p– 3s3p3d transitions in the 180–223 Å wavelength range. These ratios are subsequently compared with observations of a solar active region, obtained during the 1995 flight of the Solar EUV Research Telescope and Spectrograph (SERTS). The vers...
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ژورنال
عنوان ژورنال: Odessa Astronomical Publications
سال: 2015
ISSN: 1810-4215
DOI: 10.18524/1810-4215.2015.28.71137