An analysis on the drift pairs observed at the Yunnan Observatory during solar cycle 22.

Details An analysis on the drift pairs observed at the Yunnan Observatory during solar cycle 22. An analysis on the drift pairs observed at the Yunnan Observatory during solar cycle 22.

Dec 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995arbei..27...52m&link_type=abstract

Astrophysics Reports, Publications of the Beijing Astronomical Observatory, No. 27, p. 52 - 57

Astronomy and Astrophysics

Astrophysics

Solar Radio Bursts: Solar Activity

Scientific paper

The drift pairs (DPs) recorded at the Yunnan Observatory from July 1990
to December 1991 by using the acousto-optical spectrometer in the
frequency range of 230 - 300 MHz are analyzed. The characteristics of
the DPs and their relationship with the optical activities is discussed.

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