Comment on “Solar wind dynamic pressure variations and transient magnetospheric signatures”
نویسندگان
چکیده
منابع مشابه
Magnetospheric cavity modes driven by solar wind dynamic pressure fluctuations
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[1] Several observational studies suggest that solar wind dynamic pressure fluctuations can drive magnetospheric ultralow‐frequency (ULF) waves on the dayside. To investigate this causal relationship, we present results from Lyon‐Fedder‐Mobarry (LFM) global, three‐dimensional magnetohydrodynamic (MHD) simulations of the solar wind–magnetosphere interaction. These simulations are driven with syn...
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ژورنال
عنوان ژورنال: Geophysical Research Letters
سال: 1989
ISSN: 0094-8276
DOI: 10.1029/gl016i010p01197