Large-scale fluctuations in the solar wind at 1 AU - 1978-1982

Details Large-scale fluctuations in the solar wind at 1 AU - 1978-1982 Large-scale fluctuations in the solar wind at 1 AU - 1978-1982

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jgr....94..177b&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 94, Jan. 1, 1989, p. 177-184.

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25

Interplanetary Magnetic Fields, Plasma Oscillations, Satellite Observation, Solar Wind, Explorer 50 Satellite, Field Strength, International Sun Earth Explorer 3, Long Term Effects, Magnetic Signatures

Scientific paper

The large-scale fluctuations in the strength of the magnetic field B and the bulk speed V at 1 AU were investigated on the basis of hourly averages of IMP 8 and ISEE 3 data compiled by Couzens and King (1986). The power spectra of the intermediate frequency fluctuations in B at 1 AU had the form of a power law with exponent 1.92 + or - 0.06 during the 1978-1982 interval. The contributions of jumps to the spectra of the large-scale fluctuations in B and V were studied for the interval from days 226 to 365, 1978, which is representative of other such intervals. Of the jumps in B, 22 percent have the signature of a forward or reverse shock.

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