Terrestrial plasmaspheric imaging by an Extreme Ultraviolet Scanner on planet‐B
Terrestrial plasmaspheric imaging by an Extreme Ultraviolet Scanner on planet‐B
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DOI：
10.1029/1999gl010732
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发表时间：
2000-01
影响因子：
5.2
通讯作者：
M. Nakamura;I. Yoshikawa;A. Yamazaki;K. Shiomi;Y. Takizawa;M. Hirahara;K. Yamashita;Y. Saito;W. Miyake
中科院分区：
文献类型：
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作者：
M. Nakamura;I. Yoshikawa;A. Yamazaki;K. Shiomi;Y. Takizawa;M. Hirahara;K. Yamashita;Y. Saito;W. Miyake
火星轨道飞行器上的极紫外（XUV）扫描仪，行星B，在地球周围的停车轨道上观察到地球等离子体。这张照片只能看到等离子体望远镜黄昏的一面。尽管如此，这是第一张从等离子体显微镜外部拍摄的图像。今后的飞行任务，如2000年美国航天局的IMAGE使命以及2003年日本的SELENE等离子体层成像望远镜，将提供关于这一区域的进一步信息。
An extreme ultraviolet (XUV) scanner on board the Mars orbiter, Planet‐B, observed the terrestrial plasmasphere while it was in a parking orbit around the earth. The image was available only for the dusk side of the plasmasphere. Nonetheless, this was the first image from the outside of the plasmasphere. Future missions, such as the NASA IMAGE mission in 2000 as well as the Japanese plasmaspheric imaging telescope on SELENE in 2003 will provide further information on this region.