Photometric measurement of cold helium ions in the magnetotail by an EUV Scanner onboard planet‐B: Evidence of the existence of cold plasmas in the near‐Earth plasma sheet

Photometric measurement of cold helium ions in the magnetotail by an EUV Scanner onboard planet‐B: Evidence of the existence of cold plasmas in the near‐Earth plasma sheet
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B 行星上的 EUV 扫描仪对磁尾中冷氦离子的光度测量:近地等离子体片中存在冷等离子体的证据

DOI:
10.1029/2000gl000100
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发表时间:
2000
影响因子:
5.2
通讯作者:
M. Nakamura
M. Nakamura
中科院分区:
地球科学1区
文献类型:
--
作者:
I. Yoshikawa;A. Yamazaki;K. Shiomi;K. Yamashita;Y. Takizawa;M. Nakamura

文献摘要

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通过使用行星B上的XUV扫描仪,首次成功地对等离子体片中的He+离子进行了光学测量。He II(304 μ m)的强度为0.02瑞利。这一结果鼓励未来通过探测He II(304 μ m)发射来对整个磁层进行成像。这也证明了等离子体片中存在冷等离子体。冷离子的存在带来了一个新的问题:它们如何在等离子体片中保持低温?
The first optical measurement of He+ ions in the plasma sheet was successful by using the XUV scanner onboard Planet‐B. The intensity of He II (304 Å) was ∼0.02 Rayleigh. This result encourages future imaging missions for the whole magnetosphere by detecting He II (304 Å) emission. This is also a proof of the existence of cold plasmas in the plasma sheet. The existence of cold ions brings a new question: How can they remain cold in the plasma sheet?