It has recently been suggested that the large scale structure of the interplanetary magnetic field can be deduced solely from solar wind speed measurements. Here it is emphasized that, in addition to speed measurements, direct measurements of the interplanetary field and indirect diagnostics such as
โฆ LIBER โฆ
Magnetically closed regions in the solar wind
โ Scribed by A. Geranios
- Publisher
- Springer Netherlands
- Year
- 1982
- Tongue
- English
- Weight
- 943 KB
- Volume
- 81
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
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