The Solar U-Burst at Metre Wavelengths-Reference-Cited by-同舟云学术

The Solar U-Burst at Metre Wavelengths

Published:1970-04 Issue:7 Volume:1 Page:316-318
ISSN:1323-3580
Container-title:Publications of the Astronomical Society of Australia
language:en
Short-container-title:Publ. Astron. Soc. Aust.

Author:

Labrum N. R.,Stewart R. T.

Abstract

The U-burst, first identified by Maxwell and Swarup and Haddock, is a type of solar radio event lasting ~ 10 s in which the frequency of the emission at first drifts rapidly downwards, then increases again. On the dynamic spectrum record the burst has the appearance of an inverted letter U.

Publisher

Cambridge University Press (CUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference9 articles.

1. Contents

2. The Speed and Acceleration of the Sources of Type III And Type V Solar Radio Bursts Over Large Distances in the Corona

3. On the Relative Position and Origin of Harmonics in the Spectra of Solar Radio Bursts of Spectral Types II And III

4. Implications of solar radio bursts for the study of the solar corona

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