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

页码：313 / 318

页数：6