Shear flow driven magnetized planetary wave structures in the ionosphere
β Scribed by G.D. Aburjania; Kh.Z. Chargazia; O.A. Kharshiladze
- Book ID
- 108158907
- Publisher
- Elsevier Science
- Year
- 2010
- Tongue
- English
- Weight
- 693 KB
- Volume
- 72
- Category
- Article
- ISSN
- 1364-6826
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π SIMILAR VOLUMES
The ambipolar di}usion equation for the height distribution of electron density in the ionospheric F1!layer is solved in the presence of neutral horizontal shear ~ow[ By using this nonstationary solution the reaction of the F1!region electron density on the evolution of atmospheric acousticΓgravity
Hydromagnetic planetary-gravity waves propagating on a B-plane through a zonal flow and transverse magnetic field are examined for instability. Such instabilities may be related to same physical phenomena in the atmospheres of the Sun and planets and in the Earth's core. It is found that the onset o