The new TeePee Tee array of the Clark Lake Radio Observatory has been used to observe the quiet Sun at 121.5, 73.8 and 26.3Mtlz. The equatorial brightness distributions at all three frequencies, and the polar brightness distributions at the two higher ones have been measured. From the observed total
Imaging observations of radio bursts at meter-decameter wavelengths
โ Scribed by Mukul R. Kundu
- Publisher
- Springer
- Year
- 1987
- Tongue
- English
- Weight
- 591 KB
- Volume
- 113
- Category
- Article
- ISSN
- 0038-0938
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โฆ Synopsis
In this article, we review some of the recent results obtained with imaging observations of the Sun at meter-decameter wavelengths, using the Clark Lake multifrequency radioheliograph. We briefly discuss the use of imaging observations to study the large scale structure of the upper corona. We discuss non-flare associated type II/type IV bursts associated with a coronal streamer disruption event associated with a slow (~ 100 Km/s) CME. We discuss meter-decameter mierobursts, which occur at coronal heights, often without any surface activity. Finally, we discuss a correlated type III burst whose emission originates almost simultaneously from two widely separated (~ I0 s Km) locations.
๐ SIMILAR VOLUMES
We present the results of a study of the evolution of 3 February, 1986 flare at meter-decameter wavelengths usir~g the two dimensional imaging observations made with the Clark Lake multifrequency radioheliograph. The flare was complex and produced various types of meter-decameter bursts. The preflar