This paper presents some results of observations of the mean magnetic field of the Sun as a star (SMMF) at the Sayan Observatory during 1982-1984. A description of the instrument is given, as well as some major points in the technique of data acquisition and treatment such as calibration, zero-level
โฆ LIBER โฆ
The mean magnetic field of the Sun: Observations at Stanford
โ Scribed by Philip H. Scherrer; John M. Wilcox; Leif Svalgaard; Thomas L. Duvall; Phil H. Dittmer; Eric K. Gustafson
- Publisher
- Springer
- Year
- 1977
- Tongue
- English
- Weight
- 827 KB
- Volume
- 54
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
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The mean photospheric magnetic field of the sun seen as a star has been compared with the interplanetary magnetic field observed with spacecraft near the earth. Each change in polarity of the mean solar field is followed about 4 89 days later by a change in polarity of the interplanetary field (sect