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
โฆ LIBER โฆ
Concerning solar sources of large-scale heliospheric disturbances
โ Scribed by V. G. Fainshtein
- Publisher
- Springer
- Year
- 1992
- Tongue
- English
- Weight
- 881 KB
- Volume
- 137
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
โฆ Synopsis
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, is ungrounded. At the same time it is argued that, under certain conditions, coronal holes are indeed able to emit eruptive flows which are capable of exciting interplanetary shock waves.
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