Flare observation of the Sun as a star by SUMER/SOHO in the hydrogen Lyman continuum

被引:18
作者
Lemaire, P
Gouttebroze, P
Vial, JC
Curdt, W
Schühle, U
Wilhelm, K
机构
[1] Univ Paris 11, CNRS, Unite Mixte, IAS, F-91405 Orsay, France
[2] Max Planck Inst Aeron, D-37191 Katlenburg Lindau, Germany
关键词
Sun : flares; Sun : UV radiation; stars : flare;
D O I
10.1051/0004-6361:20034405
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
During the execution of the programme "Sun as a star", while the SUMER (Solar Ultraviolet Emission of Emitted Radiation)/SOHO (SOlar and Heliospheric Observatory) slit was collecting the scattered radiation from the telescope mirror far away from the solar disk image, a class X5.3/3b flare erupted on the solar disk, on 25 August 2001. During the first phase of the flare a relative increase of a few percent was detected at the head of the hydrogen Lyman continuum. After correction from the instrumental parameters, the relative signal increase is 70% at the head of the Lyman continuum (910 Angstrom), and 190% in the C II 904 Angstrom multiplet. Accounting for the area of the flare region, the local increase of the radiance of the Lyman continuum and of the C II lines is estimated to be a factor of several thousands. We compare this result with other solar observations and models.
引用
收藏
页码:737 / 742
页数:6
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