On the solar white-light high resolution observations from space

被引:4
作者
Veselovsky, I. S. [1 ]
Koutchmy, S.
机构
[1] Moscow MV Lomonosov State Univ, Inst Nucl Phys, Moscow 199992, Russia
[2] Russian Acad Sci, Inst Space Res, IKI, Moscow 117997, Russia
[3] CNRS, Inst Astrophys Paris, F-75014 Paris, France
来源
PARTICLE ACCELERATION, SPACE PLASMA PHYSICS, SOLAR RADIATION AND THE EARTH'S ATMOSPHERE AND CLIMATE | 2006年 / 37卷 / 08期
关键词
sun; solar activity; total solar irradiance variations; white-light flare;
D O I
10.1016/j.asr.2005.09.023
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Absolutely calibrated telescopic observations of the Sun in white-light with a sufficiently high space-time resolution from space have not been regularly performed. They are needed to resolve several important problems in the solar physics. Contributions of different morphological features to the total solar irradiance variations in the broad range of time scales from seconds up to many years can be definitely established in this manner for the first time. The quantitative role of the white-light emission in the overall energy balance of flares and eruptions on the Sun can be evaluated. More adequate theoretical models of corresponding processes on the Sun can be constructed using this new data. (c) 2006 Published by Elsevier Ltd on behalf of COSPAR.
引用
收藏
页码:1576 / 1582
页数:7
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