Electron Temperature of Solar Flares Derived from Helium-Like Sulphur Lines

Details Electron Temperature of Solar Flares Derived from Helium-Like Sulphur Lines Electron Temperature of Solar Flares Derived from Helium-Like Sulphur Lines

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997pasj...49..115y&link_type=abstract

Publications of the Astronomical Society of Japan, v.49, p.115-121.

Astronomy and Astrophysics

Astronomy

8

Sun: Corona, Sun: Flares, Sun: Spectra, Sun: X-Rays

Scientific paper

The maximum temperatures and emission measures reached in solar flares were obtained from helium-like sulphur lines, which were observed by the Bragg Crystal Spectrometer on board Yohkoh. A very weak dependence of the maximum temperature against the soft X-ray intensity was found. Similar multi-thermal characteristics prevailed in flares irrespective of the flare intensity, suggesting that the solar flare is a homogeneous phenomenon in the solar atmospheres.

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