ИСТИНА |
Войти в систему Регистрация |
|
ИПМех РАН |
||
The scaling of Hot Jupiter's magnetospheres, containing magnetodisks, is considered for different values of the intrinsic planetary magnetic dipole moment, different orbital distances, and parameters of the stellar wind. The paraboloid model of a planetary magnetosphere is used for this study. In all cases the presence of magnetodisk results in larger magnetospheres, than those caused by just a planetary magnetic dipole alone.