NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
The polar capsAccording to the most common definition, the 'polar cap' is the region bounded by the average or statistical auroral oval. Studies of the effects of the interplanetary magnetic field (IMF) on various upper atmospheric phenomena are reviewed. The Antarctic region and the Arctic region represent an area for such investigations. Particular attention is given in this paper to those observations in the highest latitude region which provide some information concerning corresponding changes of the internal structure of the magnetosphere. A definition and working definition of the polar cap are considered along with the IMF and magnetospheric models, the entry of solar energetic electrons, statistical studies regarding the aurora, individual events, polar cap arcs, the cusp aurora, auroral electron precipitation, convection, ionospheric currents and field-aligned currents, the ionosphere, the thermosphere, polar rain, polar wind, and hopping motions of heavy ions.
Document ID
19860051614
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Akasofu, S.-I.
(Alaska, University Fairbanks, United States)
Date Acquired
August 12, 2013
Publication Date
December 1, 1985
Publication Information
Publication: National Institute of Polar Research, Memoirs, Special Issue
Issue: 38 D
ISSN: 0386-0744
Subject Category
Geophysics
Accession Number
86A36352
Funding Number(s)
CONTRACT_GRANT: NSG-7447
CONTRACT_GRANT: NSF ATM-83-12515
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available