Spectral-temporal peculiarities of the microwave emission preceding geoeffective coronal mass ejections

Data on the complex of wave and spectral phenomena in the sporadic microwave emission that are associated with the formation and initial propagation of coronal mass ejections (CMEs) in the solar atmosphere are presented. Their characteristic time interval extends from 2–3 days preceding the event to...

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Veröffentlicht in:Geomagnetism and Aeronomy 2009-12, Vol.49 (8), p.1133-1136
Hauptverfasser: Fridman, V. M., Sheiner, O. A.
Format: Artikel
Sprache:eng
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Zusammenfassung:Data on the complex of wave and spectral phenomena in the sporadic microwave emission that are associated with the formation and initial propagation of coronal mass ejections (CMEs) in the solar atmosphere are presented. Their characteristic time interval extends from 2–3 days preceding the event to the time of CME recording on coronagraphs.
ISSN:0016-7932
1555-645X
0016-7940
DOI:10.1134/S0016793209080192