Spectral characteristics of a 10 ms coronal oscillation

Details Spectral characteristics of a 10 ms coronal oscillation Spectral characteristics of a 10 ms coronal oscillation

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cha%26a..17..296x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 17, Issue 3, p. 296-301.

Astronomy and Astrophysics

Astrophysics

Sun-Corona-Radio Spectrum

Scientific paper

The high-resolution radio-frequency spectrograph of Yunnan Observatory detected an oscillation with changing periods on the order of 10 ms, with a bandwidth of about 10 MHz, superposed on a radio emission which lasted some 500 ms. Corresponding burst can be found in the solar radio records of Weissenau, Germany. The Space Environment Service Center in USA also published a total intensity at 245 MHz obtained at the same time. An Hα bright spot was also identified in our series of Hα photographs.

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