Anomalous Cosmic Rays

被引:9
作者
Cummings, Alan C. [1 ]
Stone, Edward C. [1 ]
机构
[1] CALTECH, Pasadena, CA 91125 USA
来源
CENTENARY SYMPOSIUM 2012: DISCOVERY OF COSMIC RAYS | 2013年 / 1516卷
关键词
cosmic rays; anomalous cosmic rays; solar wind termination shock; PARTICLE-ACCELERATION; COMPONENT; RECONNECTION; NITROGEN; OXYGEN;
D O I
10.1063/1.4792547
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Anomalous cosmic rays (ACRs) first started showing up in observations 40 years ago. Within a few years a paradigm was developed to explain their origin: they begin their life as interstellar neutral atoms that drift into the heliosphere, become singly ionized by charge-exchange with a solar wind ion or by photoionization, are picked up by the expanding solar wind, and accelerated to the observed energies by diffusive shock acceleration at the solar wind termination shock. This paradigm became widely accepted and withstood the tests of further observations until 16 December 2004, when Voyager 1 crossed the termination shock and didn't find their source. In August 2007, Voyager 2 crossed the termination shock and also did not find the source location of ACRs. Clearly, the source location was not at the termination shock where the two Voyagers crossed. Alternative models have been proposed with acceleration elsewhere on the shock or by other acceleration processes in the heliosheath. We discuss the latest observations of ACRs from the Voyager spacecraft and hopefully shed more light on this ongoing puzzle.
引用
收藏
页码:97 / 101
页数:5
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