The Mechanism involved in the Reversals of the Sun's Polar Magnetic Fields
โ Scribed by C.J. Durrant; J.P.R. Turner; P.R. Wilson
- Book ID
- 111612005
- Publisher
- Springer
- Year
- 2004
- Tongue
- English
- Weight
- 704 KB
- Volume
- 222
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
The magnetic field strength within the polar caps of the Sun is an important parameter for both the solar activity cycle and for our understanding of the interplanetary magnetic field. Measurements of the line-of-sight component of the magnetic field generally yield 0.1 to 0.2 mT near times of sunsp
Observations of the magnetic fields in the polar regions of the Sun are presented for the period 1960-1971. At the start of this interval the fields atthe two poles were consistently of opposite sign and averaged around 1 G. Early in 1961 the field in the south decreased suddenly and the field in th
Regarding new bipolar magnetic regions as sources of flux, we have simulated the evolution of the radial component of the solar photospheric magnetic field during 1976-1984 and derived the corresponding evolution of the line-of-sight polar fields as seen from Earth. The observed timing and strength