Interplanetary magnetic flux - Measurement and balance

Details Interplanetary magnetic flux - Measurement and balance Interplanetary magnetic flux - Measurement and balance

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....97..171m&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 97, Jan. 1, 1992, p. 171-177. Research sponsored by DOE.

Physics

32

Interplanetary Magnetic Fields, Magnetic Flux, Solar Wind, Approximation, Magnetic Measurement, Satellite Observation

Scientific paper

A new method for determining the approximate amount of magnetic flux in various solar wind structures in the ecliptic (and solar rotation) plane is developed using single-spacecraft measurements in interplanetary space and making certain simplifying assumptions. The method removes the effect of solar wind velocity variations and can be applied to specific, limited-extent solar wind structures as well as to long-term variations. Over the 18-month interval studied, the ecliptic plane flux of coronal mass ejections was determined to be about 4 times greater than that of HFDs.

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