Solar Mass Ejection Imager (SMEI) observations of coronal mass ejections (CMEs) in the heliosphere

被引：57

作者：

Webb, D. F.

Mizuno, D. R.

Buffington, A.

Cooke, M. P.

Eyles, C. J.

Fry, C. D.

Gentile, L. C.

Hick, P. P.

Holladay, P. E.

Howard, T. A.

Hewitt, J. G.

Jackson, B. V.

Johnston, J. C.

Kuchar, T. A.

Mozer, J. B.

Price, S.

Radick, R. R.

Simnett, G. M.

Tappin, S. J.

机构：

[1] Univ Calif San Diego, CASS, La Jolla, CA 92093 USA

[2] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[3] Explorat Phys Int Inc, Huntsville, AL USA

[4] Boston Coll, Inst Sci Res, Chestnut Hill, MA 02167 USA

[5] Air Force Res Lab, Space Vehicles Directorate, Hanscom AFB, MA USA

[6] Montana State Univ, Dept Phys, Bozeman, MT 59717 USA

[7] Air Force Res Lab, Space Vehicles Directorate, Sunspot, NM USA

来源：

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | 2006年 / 111卷 / A12期

关键词：

D O I：

10.1029/2006JA011655

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The Solar Mass Ejection Imager (SMEI) on the Coriolis spacecraft has been obtaining white light images of nearly the full sky every 102 minutes for three years. We present statistical results of analysis of the SMEI observations of coronal mass ejections (CMEs) traveling through the inner heliosphere; 139 CMEs were observed during the first 1.5 years of operations. At least 30 of these CMEs were observed by SMEI to propagate out to 1 AU and beyond and were associated with major geomagnetic storms at Earth. Most of these were observed as frontside halo events by the SOHO LASCO coronagraphs.

引用

页数：19

共 50 条

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