First solar EUV irradiances obtained from SOHO by the CELIAS/SEM

被引:207
作者
Judge, DL [1 ]
McMullin, DR
Ogawa, HS
Hovestadt, D
Klecker, B
Hilchenbach, M
Mobius, E
Canfield, LR
Vest, RE
Watts, R
Tarrio, C
Kuhne, M
Wurz, P
机构
[1] Univ So Calif, Dept Phys & Astron, Los Angeles, CA 90089 USA
[2] Univ So Calif, Ctr Space Sci, Los Angeles, CA 90089 USA
[3] Max Planck Inst Extraterr Phys, D-85740 Garching, Germany
[4] Univ New Hampshire, Durham, NH 03824 USA
[5] Natl Inst Stand & Technol, Phys Lab, Gaithersburg, MD 20899 USA
[6] Phys Tech Bundesanstalt, D-10587 Berlin, Germany
[7] Univ Bern, Inst Phys, CH-3012 Bern, Switzerland
关键词
D O I
10.1023/A:1004929011427
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The first results obtained with the Solar EUV Monitor (SEM), part of the Charge, Element, and Isotope Analysis System (CELIAS) instrument, aboard the SOlar and Heliospheric Observatory (SOHO) satellite are presented. The instrument monitors the full-disk absolute value of the solar He II irradiance at 30.4 nm, and the full-disk absolute solar irradiance integrated between 0.1 nm and 77 nm. The SEM was first turned on December 15, 1995 and obtained 'first light' on December 16, 1995. At this time the SOHO spacecraft was close to the L-1 Lagrange point, 1.5 x 10(6) km from the Earth towards the Sun. The data obtained by the SEM during the first four and a half months of operation will be presented. Although the period of observation is near solar minimum, the SEM data reveal strong short-term solar irradiance variations in the broad-band, central image channel, which includes solar X-ray emissions.
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页码:161 / 173
页数:13
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