Relevance of plasma and neutral wind velocities to the topology and the excitation of modes for the onset of the equatorial spread F

Authors
Citation
B. Basu et B. Coppi, Relevance of plasma and neutral wind velocities to the topology and the excitation of modes for the onset of the equatorial spread F, J GEO R-S P, 104(A1), 1999, pp. 225-231
Citations number
15
Categorie Soggetti
Space Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
104
Issue
A1
Year of publication
1999
Pages
225 - 231
Database
ISI
SICI code
0148-0227(19990101)104:A1<225:ROPANW>2.0.ZU;2-M
Abstract
A theoretical model for the onset of the equatorial spread F (ESF) is intro duced that considers all the effects of the electric fields that are presen t together with the effects of the neutral wind velocity, of gravity, and o f the density gradient. These impose well-defined topological constraints o n the modes that can be excited. The horizontal (east-west) ion velocity is shown to be one of the key factors for the intrinsic vertical localization of modes that are driven unstable by the effective vertical gravity (inclu ding the E field contribution). The thickness of the layer of localization is related to the Vertical gradient of the ion horizontal velocity, of the neutral wind velocity, and of the ion-neutral collision frequency. The "hor izontal gravity" resulting from the difference between the horizontal ion a nd neutral velocities is shown to not be a driving factor for the instabili ty, under realistic conditions when the eastward electric field is included in the analysis, but to have an important influence on the mode topology ( vertical profile). An explicit analytical solution is found for the relevan t dispersion equation, which includes, in particular, the contribution of a vertical ion velocity. The mode vertical profile under conditions that are shown to be realistic is found. It is suggested that the necessary conditi ons for the intrinsic localization of the modes determine the onset of the ESF. The mode ballooning structure, along the magnetic held, including the effect of the plasma finite resistivity is also described.