The far-side solar magnetic index

被引：3
|
作者：
Hernandez, Irene Gonzalez [1 ]
Jain, Kiran [1 ]
Tobiska, W. Kent [2 ]
Hil, Frank [1 ]
机构：
[1] Natl Solar Observ, Tucson, AZ 85719 USA
[2] Space Environm Technol, Space Weatehr Div, Pacific Palisades, CA 90272 USA
来源：
GONG-SOHO 24: A NEW ERA OF SEISMOLOGY OF THE SUN AND SOLAR-LIKE STARS | 2011年 / 271卷
关键词：
IRRADIANCE;
D O I：
10.1088/1742-6596/271/1/012028
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Several magnetic indices are used to model the solar irradiance and ultimately to forecast it. However, the observation of such indices are generally limited to the Earth-facing hemisphere of the Sun. Seismic maps of the far side of the Sun have proven their capability to locate and track medium-large active regions at the non-visible hemisphere. We present here the possibility of using the average signal from these seismic far-side maps as a proxy to the non-visible solar activity which can complement the current front-side solar activity indices.
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页数：4
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