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Observation and identification of metre wave “blips”

Authors
Journal
Chinese Astronomy and Astrophysics
0275-1062
Publisher
Elsevier
Publication Date
Volume
18
Issue
2
Identifiers
DOI: 10.1016/0275-1062(94)90105-8
Keywords
  • Solar Radio Emission-Metre Wave Bursts-Blips

Abstract

Abstract 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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