Physics
Scientific paper
May 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.2781s&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 89, May 1, 1984, p. 2781-2787.
Physics
5
Geomagnetic Pulsations, Radio Emission, Very Low Frequencies, Correlation, Electron Precipitation, Ionospheric Currents, Magnetic Variations
Scientific paper
The correlations between the periodic VLF emissions and the magnetic pulsations with a period of approximately 5.6 s observed at Syowa Station, Antarctica, are examined. One-to-one correlation phenomena between the periodic VLF emissions and the magnetic pulsations were observed in the late afternoon of August 8, 1981, from 1420 to 1640 UT. At the level of the ISIS 2 satellite (altitude, aproximately 1400 km), the periodic emissions exhibited a one-to-one correspondence with the periodic emissions observed at Syowa in the wide latitude range from L approximately 3.5 to L approximately 14.0 and also in the region about two hours away from Syowa in magnetic local time. From the ground data, the intensity of the H component of magnetic pulsations associated with the periodic VLF emissions is found to be approximately 0.02 nT, about five times larger than that of the D component of magnetic pulsations.
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