A COMPARISON OF ENERGETIC STORM PROTONS TO HALO PROTONS

被引：21

作者：

KAHLER, SW

机构：

[1] Space Sciences Laboratory, University of California, Berkeley, Calif.

来源：

SOLAR PHYSICS | 1969年 / 8卷 / 01期

关键词：

D O I：

10.1007/BF00150668

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Satellite observations of solar proton events with a 'halo' structure or an energetic storm proton event and an SSC are studied. It is pointed out that some SSC events are associated with a decrease in the few MeV cosmic ray fluxes while most are associated with a flux increase. The properties of halo protons and energetic storm protons are compared. It is hypothesized that the two events are similar in origin. The propagation mode of storm particles is discussed. Evidence is presented for a solar, rather than interplanetary origin of storm protons. © 1969 D. Reidel Publishing Company.

引用

页码：166 / &

共 31 条

[1] STRUCTURE OF SOLAR PLASMA FLOW GENERATED BY SOLAR FLARES [J].