Soft X-ray Feature in Active Regions Associated with Meter Wavelength Solar Radio Emission

Details Soft X-ray Feature in Active Regions Associated with Meter Wavelength Solar Radio Emission Soft X-ray Feature in Active Regions Associated with Meter Wavelength Solar Radio Emission

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994kofu.symp..417w&link_type=abstract

In: Proceedings of Kofu Symposium, Kofu, Japan, Sept. 6-10, 1993, p.417-420.

Physics

1

Scientific paper

Solar radio bursts in meter wavelength are emitted associated with disturbances in the solar corona. Interferometers have been used to observe the structure of radio sources. However, it is difficult to get details of solar radio sources in meter-wave range because of its long wavelength. Yohkoh has observed almost the same height range of the solar corona, by the soft X-ray telescope (SXT) with high resolution, as meter-wave does. Several large meter-wave bursts have been observed in Hiraiso (N36.37 E140.63) with Yohkoh. An intense and long lasting metric continuum emission, observed after the M4.2/2N flare (S16W28) in NOAA7056 at 0127 UT on 1992 February 17, is reported here.

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