globalchange  > 气候减缓与适应
DOI: 10.1002/2017JA024860
Scopus记录号: 2-s2.0-85045836221
论文题名:
Solar Wind Properties During Juno's Approach to Jupiter: Data Analysis and Resulting Plasma Properties Utilizing a 1-D Forward Model
作者: Wilson R.J.; Bagenal F.; Valek P.W.; McComas D.J.; Allegrini F.; Ebert R.W.; Kim T.K.; Kurth W.S.; Szalay J.R.; Thomsen M.F.
刊名: Journal of Geophysical Research: Space Physics
ISSN: 21699380
出版年: 2018
卷: 123, 期:4
起始页码: 2772
结束页码: 2786
语种: 英语
英文关键词: JADE ; Juno ; solar ; upstream ; wind
英文摘要: The Jovian Auroral Distributions Experiment ion sensor (JADE-I) on board the National Aeronautics and Space Administration's Juno mission measured solar wind ions for ≈40 days prior to the spacecraft's arrival at Jupiter, simultaneous with numerous telescope observations of the Jovian aurora. JADE-I is a thermal plasma time-of-flight instrument designed to measure Jovian auroral and magnetospheric ions. This study provides a solar wind parameter data set for the approach phase that may be used in coordinated studies with remote measurements of the Jovian aurora, to compare with models that propagate solar wind conditions from Earth and to apply to Jovian bow shock or magnetopause models. While multiple bow shock crossings were predicted during Juno's approach, there was only one observed suggesting a compressed magnetosphere that was shrinking as Juno approached. However, the calculated ram pressure at the bow shock was near the median value of those 40 days, rather than being in an upper percentile. ©2018. American Geophysical Union. All Rights Reserved.
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/114188
Appears in Collections:气候减缓与适应

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作者单位: Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, United States; Southwest Research Institute, San Antonio, TX, United States; Department of Physics and Astronomy, University of Texas at San Antonio, San Antonio, TX, United States; Department of Astrophysical Sciences, Princeton University, Princeton, NJ, United States; Department of Physics and Astronomy, University of Iowa, Iowa City, IA, United States; Planetary Science Institute, Tucson, AZ, United States

Recommended Citation:
Wilson R.J.,Bagenal F.,Valek P.W.,et al. Solar Wind Properties During Juno's Approach to Jupiter: Data Analysis and Resulting Plasma Properties Utilizing a 1-D Forward Model[J]. Journal of Geophysical Research: Space Physics,2018-01-01,123(4)
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