SOLAR ENERGETIC PARTICLE 3He-RICH EVENTS FROM THE NEARLY QUIET SUN IN 2007-2008

被引:23
|
作者
Mason, G. M. [1 ]
Nitta, N. V. [2 ]
Cohen, C. M. S. [3 ]
Wiedenbeck, M. E. [4 ]
机构
[1] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[2] Lockheed Martin Solar & Astrophys Lab, Palo Alto, CA 94304 USA
[3] CALTECH, Pasadena, CA 91125 USA
[4] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
关键词
acceleration of particles; Sun: abundances; Sun: flares; Sun: particle emission; ELECTRON ACCELERATION; MAGNETIC-FIELDS; SOURCE REGIONS; FLARES; HELIOSPHERE; CONNECTION; WAVES; WIND; ACE;
D O I
10.1088/0004-637X/700/1/L56
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We have used Advanced Composition Explorer instruments to survey the period 2007 March through the end of 2008 for He-3-rich solar energetic particle (SEP) events occurring during near solar minimum conditions. Four events were found, all associated with single solar active regions in the western hemisphere. They all show He-3:He-4 ratios of a few percent (i.e., greater than or similar to 100 times solar system abundances), low intensities, and spectra extending up to at least 1 MeV nucleon(-1). Two events, on 2008 February 4 and 2008 June 16, were devoid of signatures associated with He-3-rich SEPs, namely they lacked associations with energetic electrons and type-III bursts. In addition, there were no clear coronal mass ejections and X-ray flare activity was very low or absent. We take this as evidence that the irreducible requirement for He-3-rich SEPs is a western hemisphere solar active region where magnetic and plasma processes preferentially energize He-3 and heavy ions.
引用
收藏
页码:L56 / L59
页数:4
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