Observation and identification of metre wave ``blips''

Details Observation and identification of metre wave ``blips'' Observation and identification of metre wave ``blips''

Apr 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cha%26a..18..222x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 18, Issue 2, p. 222-229.

Astronomy and Astrophysics

Astrophysics

Solar Radio Emission-Metre Wave Bursts-Blips

Scientific paper

High time-resolution (10ms), high frequency-resolution (0.5MHz) observations with the Yunnan Observatory spectrograph have led to the identification of narrow-band, short-duration, rapid frequency drift bursts in metre waves. It is a new type of metre wave bursts, different from the classical Type-III bursts, the spikes, or the Type-I bursts. Its features are similar to those of the ``blips'' in decimetre waves.

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