Physics
Scientific paper
Nov 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996r%26qe...39.1006z&link_type=abstract
Radiophysics and Quantum Electronics, Volume 39, Issue 11-12, pp. 1006-1010
Physics
Scientific paper
The method of imaging XUV spectroscopy was used to study plasma in the transition layer and inner corona of the Sun with temperatures 105 107 K in the TEREK and RES experiments on board KORONAS-I. The observations were carried out in the period from March 12 to July 5, 1994. The spectral images and their correlation with the YOHKOH X-ray images and groundbased observations are important for the study of the physical conditions and modeling of the bulk processes in the quiet Sun plasma, including active regions, corona holes, and overlimb structures.
Ignatiev Pavel A.
Klepikov Yu. V.
Korneev Valeri
Krutov Viktor V.
Kuzin Sergei V.
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