XUV observations of solar corona in the spirit experiment on board the CORONAS-F satellite

被引:17
|
作者
Zhitnik, I
Kuzin, S
Afanas'ev, A
Bugaenko, O
Ignat'ev, A
Krutov, V
Mitrofanov, A
Oparin, S
Pertsov, A
Slemzin, V
Sukhodrev, N
Urnov, A
机构
[1] RAS, PN Lebedev Phys Inst, Moscow 119991, Russia
[2] Russian Acad Sci, Inst Terr Magnetism Ionosphere & Radio Wave Propa, Troitsk 142092, Moscow Region, Russia
[3] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia
来源
HELIOSPHERE AT SOLAR MAXIMUM | 2003年 / 32卷 / 04期
关键词
D O I
10.1016/S0273-1177(03)00351-X
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The images of the solar corona from the limb out to the distance of about 5 solar radii have been obtained for the first time in the XUV narrow spectral bands and monochromatic lines in the current experiment SPIRIT (SPectroheliographIc soft X-Ray Imaging Telescope). This paper presents the examples of images for the Sun's "quiet" atmosphere as well. as for some transient and eruptive events in the corona to illustrate the performance of the instrumentation and to point out the way for future studies. The data obtained will be used for diagnostic purposes and modeling of solar wind acceleration, coronal plasma structures and various active phenomena in the solar corona. (C) 2003 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:473 / 477
页数:5
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