NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Fluctuating magnetic fields in the magnetosphere. II - ULF waves.At the present time the existing satellite observations of ULF waves suggest that the level of geomagnetic activity controls the types of waves which occur within the magnetosphere. Consequently, we consider separately quiet times, times of magnetospheric substorms, and times of magnetic storms. Within each of these categories, there are distinctly different wave modes distinguished by their polarization: either transverse or parallel to the ambient field. In addition, these wave phenomena occur in distinct frequency bands. In terms of the standard nomenclature of ground micropulsation studies ULF wave types observed in the magnetosphere include quiet time transverse - Pc 1, Pc 3, Pc 4, Pc 5; quiet time compressional - Pc 1 and Pi 1; substorm compressional Pi 1 and Pi 2; storm transverse - Pc 1; storm compressional Pc 4, 5.
Document ID
19720059236
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Mcpherron, R. L.
Russell, C. T.
Coleman, P. J., Jr.
(California, University Los Angeles, Calif., United States)
Date Acquired
August 6, 2013
Publication Date
July 1, 1972
Publication Information
Publication: Space Science Reviews
Volume: 13
Subject Category
Geophysics
Report/Patent Number
NSSDC-ID-68-014A-15-OS
NSSDC-ID-66-049A-11-OS
NSSDC-ID-68-014A-14-PS
Accession Number
72A42902
Funding Number(s)
CONTRACT_GRANT: NAS5-9098
CONTRACT_GRANT: NGL-05-007-004
CONTRACT_GRANT: NSF GA-28907
Distribution Limits
Public
Copyright
Other

Available Downloads

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