RELATION BETWEEN CORONAL mm-WAVE SOURCES, NOISE STORMS, AND CMEs
Elsevier, 1992
Online
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Zugriff:
Coronal millimeter-wave sources (CMMSs) centered at heights in the solar atmosphere of the order of 100000 km above the photospheric level have been observed for more than ten years at the Metsahovi Radio Research Station of the Helsinki University of Technology. The CMMSs appear to form a special class of long-duration post-flare emission although their relationship to single flares is not always clearly established. There is an interesting relation to gradual microwave bursts and noise storms, and also to soft X-ray long-duration events (LDEs) and coronal mass ejections (CMEs). Results of these findings are discussed and consequences for the physical interpretation outlined.
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RELATION BETWEEN CORONAL mm-WAVE SOURCES, NOISE STORMS, AND CMEs
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Autor/in / Beteiligte Person: | Hildebrandt, J. ; Krüger, A. ; Urpo, S. ; Böhme, A. |
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Veröffentlichung: | Elsevier, 1992 |
Medientyp: | unknown |
DOI: | 10.1016/b978-0-08-042049-3.50132-0 |
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