Elemental abundances of the bulk solar wind: Analyses from genesis and ACE

被引：53
|
作者：
Reisenfeld, D. B.
Burnett, D. S.
Becker, R. H.
Grimberg, A. G.
Heber, V. S.
Hohenberg, C. M.
Jurewicz, A. J. G.
Meshik, A.
Pepin, R. O.
Raines, J. M.
Schlutter, D. J.
Wieler, R.
Wiens, R. C.
Zurbuchen, T. H.
机构：
[1] Univ Montana, Dept Phys & Astron, Missoula, MT 59812 USA
[2] CALTECH, Pasadena, CA 91125 USA
[3] Univ Montana, Dept Phys, Missoula, MT 59812 USA
[4] ETH, Zurich, Switzerland
[5] Washington Univ, Dept Phys, St Louis, MO 63130 USA
[6] Arizona State Univ, Ctr Meteorite Studies, Tempe, AZ 85287 USA
[7] Univ Michigan, Ann Arbor, MI 48109 USA
[8] Los Alamos Natl Lab, Los Alamos, NM USA
来源：
SPACE SCIENCE REVIEWS | 2007年 / 130卷 / 1-4期
关键词：
Sun; etc;
D O I：
10.1007/s11214-007-9215-1
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Analysis of the Genesis samples is underway. Preliminary elemental abundances based on Genesis sample analyses are in good agreement with in situ-measured elemental abundances made by ACE/SWICS during the Genesis collection period. Comparison of these abundances with those of earlier solar cycles indicates that the solar wind composition is relatively stable between cycles for a given type of flow. ACE/SWICS measurements for the Genesis collection period also show a continuum in compositional variation as a function of velocity for the quasi-stationary flow that defies the simple binning of samples into their sources of coronal hole (CH) and interstream (IS).
引用
收藏
页码：79 / 86
页数：8
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