Temperature structure of active regions deduced from the helium-like sulphur lines     

Tetsuya Watanabe  Hirohisa Haka  Toshifumi Shimizu  Eijiro Hiei  Robert D. Bentley  James Lang  Kenneth J. H. Phillips  C. David Pike  Andrzej Fludra  Barbara J. I. Bromage  John T. Mariska 《Solar physics》1995,157(1-2):169-184

Solar active-region temperatures have been determined from the full-Sun spectra of helium-like sulphur (Sxv) observed by the Bragg Crystal Spectrometer on board theYohkoh satellite. The average temperature deduced from Sxv is demonstrated to vary with the solar activity level: A temperature of 2.5 × 10⁶ K is derived from the spectra taken during low solar activity, similar to the general corona, while 4 × 10⁶ K is obtained during a higher activity phase. For the latter, the high-temperature tail of the differential emission measure of active regions is found most likely due to the superposition of numerous flare-like events (micro/nano-flares).  相似文献