Ion distribution functions in the vicinity of comet Giacobini‐Zinner
作者:
T. E. Cravens,
期刊:
Geophysical Research Letters
(WILEY Available online 1986)
卷期:
Volume 13,
issue 3
页码: 275-278
ISSN:0094-8276
年代: 1986
DOI:10.1029/GL013i003p00275
数据来源: WILEY
摘要:
Photoionization of neutral molecules in the coma surrounding a comet produces heavy ions which contaminate and mass‐load the solar wind. Cometary ion distribution functions in the vicinity of comet Giacobini‐Zinner (G/Z) are calculated using a Monte Carlo method. The distribution function calculated behind the shock has both cold (≈ 2 keV) and hot (≈ 40 keV) com
点击下载:
PDF
(368KB)
返 回