Geomagnetic response at low latitude to continuous solar wind pressure variations during northward interplanetary magnetic field

Details Geomagnetic response at low latitude to continuous solar wind pressure variations during northward interplanetary magnetic field Geomagnetic response at low latitude to continuous solar wind pressure variations during northward interplanetary magnetic field

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999jgr...10419923f&link_type=abstract

Journal of Geophysical Research, Volume 104, Issue A9, p. 19923-19930

Physics

21

Magnetospheric Physics: Magnetospheric Configuration And Dynamics, Magnetospheric Physics: Solar Wind/Magnetosphere Interactions

Scientific paper

A study of the geomagnetic field response to a series of continuous solar wind pressure variations has been performed at a low-latitude station during interplanetary events characterized by stable northward magnetic field conditions. The geomagnetic field H component responds well to the solar wind pressure changes on a timescale of few minutes. The amplitude of the geomagnetic field response is found to depend on local time, showing greater values around local noon and midnight.

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