NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Quiet time observations of equatorially trapped megaelectronvolt radiation belt ions with nuclear charge Z greater than or equal to 4Data from the equatorial satellite Explorer 45 were used to study ion fluxes during the geomagnetically quiescent period June 1-15, 1972. A heavy-ion solid-state ion detector system obtained count rates close to the equatorial plane in the energy passband 1.82-4.8 MeV per ion during a single satellite pass through the radiation belts. Fluxes of these ions are interpreted as oxygen ions and are found to maximize in the L shell range 3-3.5 with peak equatorially mirroring flux of 0.38 ions/(sq cm s sr keV). This peak is not as sharply confined in L shell as is the helium ion peak.
Document ID
19780068625
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Spjeldvik, W. N.
(National Oceanic and Atmospheric Administration Boulder, CO, United States)
Fritz, T. A.
(NOAA, Space Environment Laboratory, Boulder Colo., United States)
Date Acquired
August 9, 2013
Publication Date
September 1, 1978
Publication Information
Publication: Journal of Geophysical Research
Volume: 83
Subject Category
Space Radiation
Accession Number
78A52534
Funding Number(s)
CONTRACT_GRANT: NASW-13952
Distribution Limits
Public
Copyright
Other

Available Downloads

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