Radial dependence of solar energetic particle events

被引：0

作者：

Kallenrode, MB ^{[1
]}

机构：

[1] Univ Osnabruck, FB Phys, D-49076 Osnabruck, Germany

来源：

PROCEEDINGS OF THE CONFERENCE SOLAR WIND 11 - SOHO 16: CONNECTING SUN AND HELIOSPHERE | 2005年 / 592卷

关键词：

solar energetic particles; interplanetary propagation; shocks; 5 MEV PROTONS; COSMIC-RAYS; ADIABATIC DECELERATION; INTERPLANETARY SHOCKS; HE-3; ENHANCEMENTS; ACCELERATION; ULYSSES; PROPAGATION; IONS; TRANSPORT;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Solar energetic particle (SEP) events have been observed from Mercury's orbit to beyond Saturn's. With increasing radial distance, the number of particle events decreases, maximum fluxes decrease, time scales increase and profiles become more rounded. Relevant observations from Helios and Ulysses will be reviewed; focus is on anisotropies, time scales, streaming-limits and invariant spectra. Implications for the current paradigm of SEP events will be discussed and SEP history will be addressed: SEP events, in particular at larger distances, cannot be regarded as isolated events but are modified by previous SEP events and other aspects of solar activity.

引用

页码：87 / 94

页数：8

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