NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Characteristics of reflected and diffuse ions upstream from the earth's bow shockThe distinction between two types of upstream ion populations is made on the basis of pronounced differences in their distribution functions. The reflected ions represent a fast beam with temperatures typically one-million to five-million K and speeds up to five times the solar wind speed. An important feature of the reflected ion distributions is their strong temperature anisotropy, with perpendicular temperature exceeding parallel temperature by a factor of two or three. In contrast, the diffuse ions occupy a much larger region of phase space, both in energy and angle; their distribution function generally has the form of a circular ridge in two dimensions and a spherical shell in three dimensions. Accordingly, their temperature is much larger (not less than about 10-million K) and their bulk speed is typically smaller than the solar wind speed.
Document ID
19810054527
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Paschmann, G.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Sckopke, N.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Papamastorakis, I.
(Max-Planck-Institut fuer extraterrestrische Physik Garching, Germany)
Asbridge, J. R.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Bame, S. J.
(Max-Planck-Inst. fuer Extraterrestrische Physik Garching, Germany)
Gosling, J. T.
(California, University Los Alamos Scientific Laboratory, Los Alamos, NM, United States)
Date Acquired
August 11, 2013
Publication Date
June 1, 1981
Subject Category
Geophysics
Accession Number
81A38931
Funding Number(s)
CONTRACT_GRANT: NASA ORDER S-50864-A
CONTRACT_GRANT: BMFT-01-OI-027-ZA/WF/WRK-2754
Distribution Limits
Public
Copyright
Other

Available Downloads

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