Exospheric solar wind charge exchange as seen by XMM-Newton

被引：7
作者：
Carter, J. A. [1 ]
Sembay, S. [1 ]
Read, A. M. [1 ]
机构：
[1] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
来源：
ASTRONOMISCHE NACHRICHTEN | 2012年 / 333卷 / 04期
基金：
英国科学技术设施理事会;
关键词：
radiation mechanism: general; solar system: general; X-rays: diffuse background; CORONAL MASS EJECTIONS; X-RAY-EMISSION;
D O I：
10.1002/asna.201211661
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We review a selection of recent papers describing solar wind charge exchange emission occurring in the Earth's exosphere as seen by the X-ray observatory XMM-Newton. We discuss the detection of this emission, the occurrence with respect to the solar cycle and solar activity, and various spectral signatures observed. We also describe a model developed to predict the X-ray signal from exospheric charge exchange as would be detected by XMM-Newton, given the upstream solar wind conditions obtained from in situ solar wind monitors. (c) 2012 WILEY-VCH Verlag GmbH&Co. KGaA, Weinheim
引用
收藏
页码：313 / 318
页数：6
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