Transmission of solar wind hydromagnetic energy into the terrestrial magnetosphere

Details Transmission of solar wind hydromagnetic energy into the terrestrial magnetosphere Transmission of solar wind hydromagnetic energy into the terrestrial magnetosphere

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988georl..15.1275s&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 15, Oct. 1988, p. 1275-1278.

Other

17

Earth Magnetosphere, Energy Transfer, Solar Terrestrial Interactions, Solar Wind, Space Plasmas, Interplanetary Magnetic Fields, Power Spectra

Scientific paper

The relationships between the IMF and hydromagnetic energy in the band 20-50 mHz, as measured on the ground near a dayside magnetopause field line, are examined quantitatively. For this band, the distribution of signal frequencies as a function of IMF magnitude has two distinct branches. In one branch, signal frequency is independent of IMF magnitude, while the other branch shows signal frequency as a linear function of IMF magnitude similar to the results of Gul'elmi (1974). The sources of these branches are discussed.

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