Parallel acceleration and transport of ions from polar ionosphere to plasma sheet

The effect of the convection electric field in accelerating ions that escape from the polar ionosphere is investigated. It is shown that at high altitudes the velocity component of the ions along the magnetic field may be increased by more than an order of magnitude. The highest velocities are acqui...

Full description

Saved in:
Bibliographic Details
Published inGeophysical research letters Vol. 13; no. 9; pp. 893 - 896
Main Author Cladis, J. B.
Format Journal Article
LanguageEnglish
Published Legacy CDMS Blackwell Publishing Ltd 01.09.1986
American Geophysical Union
Subjects
Online AccessGet full text

Cover

Loading…
More Information
Summary:The effect of the convection electric field in accelerating ions that escape from the polar ionosphere is investigated. It is shown that at high altitudes the velocity component of the ions along the magnetic field may be increased by more than an order of magnitude. The highest velocities are acquired by ions that escape from the region of the ionosphere that is connected along magnetic field lines to the dayside cusps. During disturbed times, ions from that region intercept the center plane of the magnetotail in one to two hours at radial distances exceeding about 6 earth radii. Investigation of the resulting O(+) properties in the center plane, viz., their locations, number densities, and energies, indicates that the polar ionosphere near the cusps is the principal source of the O(+) observed in the plasma sheet. Moreover, a study of the ion motion at quiet and disturbed times indicates that the increase of O(+) in the plasma sheet with increasing AE values (Lennartsson and Shelley, 1986) is due mainly to an increase in the source of O(+) rather than alteration of its transport path.
Bibliography:ark:/67375/WNG-BSDHVQGV-B
istex:C99E332E7B09481CF4C3A0C4A5A78ACC785C078E
ArticleID:6L6235
CDMS
Legacy CDMS
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ObjectType-Article-2
ObjectType-Feature-1
ISSN:0094-8276
1944-8007
DOI:10.1029/GL013i009p00893