Autor: |
Z. A. Sokhadze, R. G. Chanishvili, J. G. Lominadze, George Chagelishvili |
Rok vydání: |
1990 |
Předmět: |
|
Zdroj: |
Symposium - International Astronomical Union. 140:395-398 |
ISSN: |
0074-1809 |
Popis: |
The simplest case of the nonlinear turbulent dynamo mechanism is proposed. It is shown that under certain conditions the generated mean magnetic field can become stronger than the small-scale one. Some manifestations (the model of Cyg X-1 bimodal behaviour, asymmetric accretion onto the magnetized rotating compact star) of this mean field are discussed. |
Databáze: |
OpenAIRE |
Externí odkaz: |
|