Relationship between field line resonance at low geomagnetic latitudes and solar wind structures

Details Relationship between field line resonance at low geomagnetic latitudes and solar wind structures Relationship between field line resonance at low geomagnetic latitudes and solar wind structures

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991georl..18.1501v&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 18, Aug. 1991, p. 1501-1503. Research supported by CNR and Ministero dell'Un

Mathematics

Logic

5

Geomagnetism, Interplanetary Magnetic Fields, Interplanetary Medium, Resonance Lines, Solar Wind, Correlation Coefficients, Diurnal Variations

Scientific paper

The link between the pulsation activity in the local resonant band at a low latitude station and the macroscale structure of the interplanetary medium has been investigated. The experimental results show a clear dependence of the amplitude of the local resonant events on the interplanetary magnetic field magnitude and a preferable occurrence in correspondence of the compression regions preceding the high velocity solar wind streams. These features appear consistent with an upstream wave source for these events.

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