Abstract
The early phases of three flares, observed by the Nobeyama Radio Heliograph, are studied. Nonthermal and thermal radio sources are identified by comparison with soft X-ray images taken by the Soft X-ray Telescope onboard the Yohkoh satellite. Two of the flares are mainly of nonthermal origin and their location coincides with one of the foot points of soft X-ray loops. Another flare has both thermal and nonthermal components which start to brighten simultaneously. This suggests that particle acceleration and plasma compression develop simultaneously.
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© 1994 Springer Science+Business Media Dordrecht
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Shibasaki, K. et al. (1994). Thermal and Nonthermal Flare Emission Observed with the Nobeyama Radio Heliograph. In: Van den Oord, G.H.J. (eds) Fragmented Energy Release in Sun and Stars. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1014-3_30
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DOI: https://doi.org/10.1007/978-94-011-1014-3_30
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4441-7
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