Diagnosing Solar Plasmas From EUV and X-Ray Emission Lines
نویسندگان
چکیده
منابع مشابه
FeXVII X-ray lines in solar coronal and laboratory plasmas
Theoretical intensities of the Fe xviiX-ray lines due to transitions 2p6 − 2p53d (near 15 Å) and 2p6 − 2p53s (near 17 Å) are presented, and compared with solar flare and active region spectra. The ratio of the 15 Å lines to the 17 Å lines is a function of temperature Te, but for solar spectra this is not of practical use because of the resonance scattering of the intense 15.015 Å line. Instead ...
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ژورنال
عنوان ژورنال: Symposium - International Astronomical Union
سال: 1990
ISSN: 0074-1809
DOI: 10.1017/s0074180900088318