Spatial and Temporal Evolution of Magnetic Loops on April 15, 1998

Details Spatial and Temporal Evolution of Magnetic Loops on April 15, 1998 Spatial and Temporal Evolution of Magnetic Loops on April 15, 1998

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..287h&link_type=abstract

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

Physics

2

Scientific paper

The first detections of subsecond type-U bursts are reported by the Beijing Astronomical Observatory using the solar radio spectrometer operating between 2.6-3.8 GHz with a time resolution of 8 msec. The spatial and temporal evolution of these loop-like structures are studied and compared with the relevant observations at optical, X-ray, and radio bands.

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