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Decrease of the first Schumann resonance frequency during solar proton events
The variations of the first‐order Schumann resonance frequency in Kola peninsula are studied for four solar proton events on November 4 and 6, 1997 and on May 2 and May 6, 1998. It is found that the frequency decreases by about 0.15 Hz during the peaks of the proton penetrations. Such a decrease is...
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Published in: | Journal of Geophysical Research 2001-09, Vol.106 (A9), p.18555-18562 |
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Main Authors: | , , , |
Format: | Article |
Language: | English |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | The variations of the first‐order Schumann resonance frequency in Kola peninsula are studied for four solar proton events on November 4 and 6, 1997 and on May 2 and May 6, 1998. It is found that the frequency decreases by about 0.15 Hz during the peaks of the proton penetrations. Such a decrease is in agreement with modeling calculations. A very intensive solar X ray burst preceding the proton flare on November 6 caused an increase of the resonance frequency. The decrease of amplitude about of 0.2 pT and the decrease of the resonance bandwidth about of 0.2 Hz are observed in the November events. |
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ISSN: | 0148-0227 2156-2202 |
DOI: | 10.1029/2000JA900118 |