Computer Science – Sound
Scientific paper
Mar 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991jgr....96.3465y&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 96, March 1, 1991, p. 3465-3470. Research supported by Gruppo Italiano di
Computer Science
Sound
11
Interplanetary Magnetic Fields, Micropulsations, Satellite Sounding, Solar Activity, Solar Wind, Annual Variations, Solar Terrestrial Interactions, Solar Wind Velocity
Scientific paper
A year-long comparison between daily averages of solar wind parameters obtained from the MIT experiment on IMP-8 and micropulsation measurements made by the Universita dell'Aquila has shown a correlation between solar wind speed and micropulsation power with peaks of the correlation coefficient greater than 0.8 in the period range from 20 to 40 s. Different behavior observed for different period bands suggests that the shorter period activity tends to precede the highest values of the solar wind speed while the longer period activity tends to persist for longer intervals within high velocity solar wind streams. A comparison with simultaneous interplanetary magnetic field measurements supports the upstream origin of the observed ground pulsations.
Lazarus Andrew J.
Vellante Massimo
Villante Umberto
Yedidia Adam B.
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