| 11. | In front of the magnetopause ( at a distance from 80 to 130 " R"
|
| 12. | A recent study shows that these waves enable incoming charged particles of solar wind to breach the magnetopause.
|
| 13. | The "'magnetopause "'is the abrupt boundary between a magnetosphere and the surrounding plasma.
|
| 14. | For planetary science, the magnetopause is the boundary between the planet s magnetic field and the solar wind.
|
| 15. | :: : Sun, solar flare, birkeland current, heliopause, magnetopause, current sheet, magnetohydrodynamics.
|
| 16. | Empirical models using real-time solar wind data can provide a real-time estimate of the magnetopause location.
|
| 17. | Research on the magnetopause is conducted using the LMN coordinate system ( which is set of axes like XYZ ).
|
| 18. | This orbit also allows us to study the boundary region of the magnetosphere as it skims the magnetopause at perigees.
|
| 19. | The magnetopause's position depends on the pressure exerted by the solar wind, which in turn depends on solar activity.
|
| 20. | The outer boundary of geospace is the magnetopause, which forms an interface between the planet's magnetosphere and the solar wind.
|