NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
On the minimum fluxes of low-energy ions (0.5 MeV/NUC - 8 MeV/NUC) at high heliospheric latitudesThe quiet-time fluxes of ions from 0.5 MeV/nuc to 7 MeV/nuc (for oxygen) have been studied for the time period between mid-1993 through the first 104 days of 1994. During this time period, Ulysses was below the heliographic current sheet. We find that at the quietest times, the ion population is dominated by the anomalous cosmic ray (ACR) component. For more active times, but still avoiding the most active time periods, the population below 3 MeV/nuc contains a CIR component as well as ACR ions.
Document ID
19950052423
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Blake, J. B.
(The Aerospace Corporation Los Angeles, CA, US, United States)
Fraenz, M.
(Max-Planck-Institut fuer Aeronomie Katlenburg-Lindau, Germany)
Keppler, E.
(Max-Planck-Institut fuer Aeronomie Katlenburg-Lindau, Germany)
Krupp, N.
(Max-Planck-Institut fuer Aeronomie Katlenburg-Lindau, Germany)
Ruess, M. K.
(Max-Planck-Institut fuer Aeronomie Katlenburg-Lindau, Germany)
Quenby, J. J.
(Imperial College London, UK, United States)
Date Acquired
August 16, 2013
Publication Date
July 1, 1995
Publication Information
Publication: Advances in Space Research
Volume: 15
Issue: 7
ISSN: 0273-1177
Subject Category
Solar Physics
Accession Number
95A84022
Funding Number(s)
CONTRACT_GRANT: JPL-958748
Distribution Limits
Public
Copyright
Other

Available Downloads

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