A NEW MECHANISM FOR POLAR PATCH FORMATION

Citation
As. Rodger et al., A NEW MECHANISM FOR POLAR PATCH FORMATION, J GEO R-S P, 99(A4), 1994, pp. 6425-6436
Citations number
40
Categorie Soggetti
Geosciences, Interdisciplinary","Astronomy & Astrophysics","Metereology & Atmospheric Sciences
Journal title
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN journal
21699380 → ACNP
Volume
99
Issue
A4
Year of publication
1994
Pages
6425 - 6436
Database
ISI
SICI code
2169-9380(1994)99:A4<6425:ANMFPP>2.0.ZU;2-1
Abstract
Polar patches are regions within the polar cap where the F-region elec tron concentration and airglow emission at 630 nm are enhanced above a background level. Previous observations have demonstrated that polar patches can be readily identified in Polar Anglo-American Conjugate Ex periment (PACE) data. Here PACE data and those from complementary inst ruments are used to show that some polar patches form in the dayside c usp within a few minutes of the simultaneous occurrence of a flow chan nel event (short-lived plasma jets approximately 2 km s-1) and azimuth al flow changes in the ionospheric convection pattern. The latter are caused by variations of the y-component of the interplanetary magnetic field. The physical processes by which these phenomena cause plasma e nhancements and depletions in the vicinity of the dayside cusp and cle ft are discussed. Subsequently, these features are transported into th e polar cap where they continue to evolve. The spatial scale of patche s when formed is usually 200-1000 km in longitude and 2-degrees-3-degr ees wide in latitude. Their motion after formation and the velocity of the plasma within the patches are the same, indicating that they are drifting under the action of an electric field. Occasionally, patches are observed to occur simultaneously in geomagnetic conjugate regions. Since some of these observations are incompatible with the presently- accepted model for patch formation involving the expansion of the high latitude convection pattern entraining solar-produced plasma, further modeling of the effects of energetic particle precipitation in the cu sp, the consequences of flow channel events on the plasma concentratio ns, and the time dependence of plasma convection as a result of interp lanetary magnetic field By changes is strongly recommended. Such studi es could be used to determine the relative importance of this new mech anism compared with the existing theory for patch formation as a funct ion of universal time and season.