Helium observation in the Martian ionosphere by an X-ray ultraviolet scanner on Mars orbiter NOZOMI
Helium observation in the Martian ionosphere by an X-ray ultraviolet scanner on Mars orbiter NOZOMI
复制标题
火星轨道飞行器 NOZOMI 上的 X 射线紫外线扫描仪对火星电离层中的氦进行观测
DOI：
10.1186/bf03352210
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发表时间：
1999
期刊：
影响因子：
--
通讯作者：
S. Chakrabarti
中科院分区：
文献类型：
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作者：
M. Nakamura;K. Yamashita;I. Yoshikawa;K. Shiomi;A. Yamazaki;S. Sasaki;Y. Takizawa;M. Hirahara;W. Miyake;Y. Saito;S. Chakrabarti
我们在火星轨道器NOZOMI（行星B）上建造了一台X射线紫外线扫描仪。该扫描仪的主要目标是来自火星大气层和电离层的He I和II辐射。这些极紫外辐射为研究火星地质历史和太阳风与火星电离层之间的相互作用提供了重要信息。XUV扫描仪将在环绕地球的停泊轨道和前往火星的转移轨道上运行，在那里将研究地球等离子体辐射和行星际辐射。
We have built an X-ray ultraviolet (XUV) scanner on board Mars orbiter NOZOMI (Planet-B). This scanner has the He I and II emissions from the Martian atmosphere and ionosphere as its main target. These EUV emissions provide important information for the study of both Martian geological history and the interaction between solar wind and the Martian ionosphere. The XUV scanner will be operated in the parking orbit around the earth and also in the transfer orbit to Mars, where the terrestrial plasmasphere and interplanetary emissions will be studied.