Physics
Scientific paper
May 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983p%26ss...31..559g&link_type=abstract
Planetary and Space Science (ISSN 0032-0633), vol. 31, May 1983, p. 559-567. Research supported by the Association of Commonweal
Physics
17
Frequency Distribution, Geomagnetic Micropulsations, Interplanetary Magnetic Fields, Magnetic Flux, Solar Activity Effects, Solar Wind, Regression Analysis, Statistical Distributions
Scientific paper
It has been suggested, in light of an apparent relationship between the frequency of Pc 3-4 geomagnetic pulsations observed in the solar wind and the strength of the IMF, that some magnetospheric Pc 3-4 pulsations have an exogenic source. A statistical reappraisal is presently given of some of the earlier results, together with newly obtained ground and solar wind pulsation data sets which suggest that, on the exclusive basis of a frequency-field strength relationship, the case for an exogenic source remains unproven. Support is nevertheless found for the frequency-field strength relationship for ground pulsations, and it is confirmed that the pulsation frequency is an imprecise predictor at best.
Green Cristina A.
Odera T. J.
Stuart W. F.
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