Recent observations demonstrate that some type II radio bursts (a) occur below the top of coronal white light loops in the early stages and (b) travel faster than white light transients when both data sources are recorded concurrently. These characteristics are examined with numerical simulations of
Coronal transients in radio and X-rays
β Scribed by Mukul R. Kundu
- Publisher
- Springer Netherlands
- Year
- 1996
- Tongue
- English
- Weight
- 728 KB
- Volume
- 243
- Category
- Article
- ISSN
- 0004-640X
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