Initial observational data and their analysis made by Hewish and Bravo (1986) are examined critically. It is shown that the conclusion drawn by them that coronal holes are solar sources of all eruptive plasma flows recorded in interplanetary space by the method of IPS-images using 900 radio sources,
Large-scale component of dynamics of the local solar sources of cm-radiation
โ Scribed by O. A. Golubchina
- Publisher
- Springer
- Year
- 1995
- Tongue
- English
- Weight
- 397 KB
- Volume
- 160
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
Observations on a grid of 900 radio sources have been used to map and to track large-scale structures in the solar wind at distances of 0.6-1.5 AU from the Sun. Most of the disturbances were shells &enhanced density followed by high-speed streams lasting for several days, although more stable eorota
The slowly varying component of solar centimeter wavelength radiation can often be attributed to thermal emission from density enhancements above an active region. This assertion is justified by the success in reproducing the observations by ray tracing calculations in appropriate coronal models. Si