On the origin of microwave type U-bursts

Details On the origin of microwave type U-bursts On the origin of microwave type U-bursts

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003a%26a...411..263a&link_type=abstract

Astronomy and Astrophysics, v.411, p.263-271 (2003)

Astronomy and Astrophysics

Astrophysics

6

Sun: Flares, Sun: Activity, Sun: Radio Radiation

Scientific paper

An analysis is made of the observations of U-type cm-bursts recorded simultaneously with high spatial (Siberian solar radio telescope) and spectral resolution (National Astronomical Observatories/Beijing spectropolarimeters). It is shown that the source positions of increasing and decreasing branches of the U-burst coincide within a few arcsec. The suggestion is made that the occurrence of the observed type U-bursts at microwave frequencies is associated with a pressure and density response to rapid heating pulses in flare loops.}

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