Generation of auroral turbulence through the magnetosphere–ionosphere coupling
The shear Alfvén waves coupled with the ionospheric density fluctuations in auroral regions of a planetary magnetosphere are modeled by a set of the reduced magnetohydrodynamic and two-fluid equations. When the drift velocity of the magnetized plasma due to the background electric field exceeds a cr...
| Asıl Yazarlar: | , , |
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| Materyal Türü: | Makale |
| Dil: | English |
| Baskı/Yayın Bilgisi: |
IOP Publishing
2016-01-01
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| Seri Bilgileri: | New Journal of Physics |
| Konular: | |
| Online Erişim: | https://doi.org/10.1088/1367-2630/aa532a |