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Cowley, S.W.H., Badman, S.V., Imber, S.M. and Milan, S.E. (2008) Comment on “Jupiter: A Fundamentally Different Magnetospheric Interaction with the Solar Wind” by D.J. McComas and F. Bagenal. Geophysical Research Letters, 35, Article No. L101010.
https://doi.org/10.1029/2007GL032645

has been cited by the following article:

• TITLE: Solar Wind Interaction with Jupiter’s Magnetosphere

  AUTHORS: Jenny Marcela Rodríguez-Gómez

  KEYWORDS: Solar Wind, Interplanetary Fast Shocks, Magnetospheres

  JOURNAL NAME: Advances in Aerospace Science and Technology, Vol.8 No.3, September 13, 2023

  ABSTRACT: 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.