Nobeyama Radioheliograph Data on Dynamics of Microwave Counterparts of Giant Post-Eruptive Soft X-ray Arches

Details Nobeyama Radioheliograph Data on Dynamics of Microwave Counterparts of Giant Post-Eruptive Soft X-ray Arches Nobeyama Radioheliograph Data on Dynamics of Microwave Counterparts of Giant Post-Eruptive Soft X-ray Arches

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..203c&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

Scientific paper

The dynamics of a number of giant post-eruptive arches in several near-the-limb events is studied using the Nobeyama Radioheliograph data at 17 GHz in comparison with observations of the Yohkoh Soft X-ray Telescope. It is found that the leading front and the brightest part of some microwave arches rise in the corona with a characteristic speed of 1--4 km/s, coinciding with that of soft X-ray arches, and lift to altitudes of at least about of 140,000 of km.

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