MLSO Mark III K-Coronameter Observations of the CME Rate from 1989-1996

被引：8

作者：

St Cyr, O. C. ^{[1
,2
]}

Flint, Q. A. ^{[2
,3
]}

Xie, H. ^{[2
]}

Webb, D. F. ^{[4
]}

Burkepile, J. T. ^{[5
]}

Lecinski, A. R. ^{[5
]}

Quirk, C. ^{[2
]}

Stanger, A. L. ^{[5
]}

机构：

[1] NASA, GSFC, Code 670, Greenbelt, MD 20771 USA

[2] Catholic Univ Amer, Dept Phys, Washington, DC 20064 USA

[3] Gustavus Adolphus Coll, St Peter, MN 56082 USA

[4] Boston Coll, Inst Sci Res, Chestnut Hill, MA 02467 USA

[5] High Altitude Observ, Boulder, CO 80301 USA

来源：

SOLAR PHYSICS | 2015年 / 290卷 / 10期

基金：

美国国家科学基金会;

关键词：

Solar corona; Coronal mass ejections; Solar activity; SOLAR MAXIMUM MISSION; MASS EJECTIONS; BRIGHTNESS VARIATIONS; SMM OBSERVATIONS; ELECTRON CORONA; CYCLE VARIATION; LASCO; POLARIMETER; SPACECRAFT; CATALOG;

D O I：

10.1007/s11207-015-0780-2

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We report here an attempt to fill the 1990 -aEuro parts per thousand 1995 gap in the CME rate using the Mauna Loa Solar Observatory's Mark III (Mk3) K-coronameter. The Mk3 instrument observed routinely several hours most days beginning in 1980 until it was upgraded to Mk4 in 1999. We describe the statistical properties of the CMEs detected during 1989 -aEuro parts per thousand 1996, and we determine a CME rate for each of those years. Since spaceborne coronagraphs have more complete duty cycles than a ground-based instrument at a single location, we compare the Mk3-derived CME rate from 1989 with the rate from the SMM C/P coronagraph, and from 1996 with the rate from the SOHO LASCO coronagraphs.

引用

页码：2951 / 2962

页数：12

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