| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1768642 | Advances in Space Research | 2005 | 5 Pages |
Abstract
It is generally assumed that magnetic fields inside interplanetary magnetic clouds and flux ropes in the solar photosphere are force-free. In order to model such fields, the solution of rot B = αB is commonly used where α = const. But comparisons of this solutions with observations show significant difference. To treat this problem,we examine the solutions with α=α0/(1+r/r0)3/2.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
E. Romashets, M. Vandas,