Solar Wind Interaction with Jupiter’s Magnetosphere  

作　　者：Jenny Marcela Rodríguez-Gómez Jenny Marcela Rodríguez-Gómez(NASA Goddard Space Flight Center, Greenbelt, USA;Physics Department, The Catholic University of America, Washington DC, USA)

机构地区：[1]NASA Goddard Space Flight Center, Greenbelt, USA [2]Physics Department, The Catholic University of America, Washington DC, USA

出　　处：《Advances in Aerospace Science and Technology》2023年第3期34-54,共21页航空科学与技术（英文）

摘　　要：This paper studies the effects of the solar wind on Jupiter’s magnetosphere. The solar wind parameters are characterized using the Michigan Solar Wind Model (mSWiM) solar wind data propagated to Jupiter from 1997 to 2016. This analysis covers almost solar cycles 23 and 24. Interplanetary fast shocks: Forward shocks (FS), Reverse shocks (RS), and solar wind dynamic pressure were obtained and analyzed during the apparent opposition periods. The fast forward (FS) shocks were predominant during this period. Generally, the solar wind dynamic pressure from FS and RS shocks follows the solar cycles 23 and 24.This paper studies the effects of the solar wind on Jupiter’s magnetosphere. The solar wind parameters are characterized using the Michigan Solar Wind Model (mSWiM) solar wind data propagated to Jupiter from 1997 to 2016. This analysis covers almost solar cycles 23 and 24. Interplanetary fast shocks: Forward shocks (FS), Reverse shocks (RS), and solar wind dynamic pressure were obtained and analyzed during the apparent opposition periods. The fast forward (FS) shocks were predominant during this period. Generally, the solar wind dynamic pressure from FS and RS shocks follows the solar cycles 23 and 24.

关 键 词：Solar Wind Interplanetary Fast Shocks MAGNETOSPHERES 

分 类 号：F41[经济管理—产业经济]