The spectrum of magnetic field irregularities in the solar corona and in interplanetary space
✍ Scribed by I.V. Chashei; A.I. Efimov; L.N. Samoznaev; M.K. Bird; M. Pätzold
- Book ID
- 108427447
- Publisher
- Elsevier Science
- Year
- 2000
- Tongue
- English
- Weight
- 597 KB
- Volume
- 25
- Category
- Article
- ISSN
- 0273-1177
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The three-dimensional structure of the solar magnetic field in the interplanetary space is inferred from a theoretical point of view. We use the magnetic field produced by a magnetic dipole rotating obliquely in vacuum. The correction for the presence of a plasma surrounding the Sun is taken into ac
Figs. la-b. An example of the weak field (a) and strong field (b) maps contained in the 'Atlas of Magnetic Fields in the Solar Corona'.