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Iron charge states observed in the solar windSolar wind measurements from the ULECA sensor of the Max-Planck-Institut/University of Maryland experiment on ISEE-3 are reported. The low energy section of approx the ULECA sensor selects particles by their energy per charge (over the range 3.6 keV/Q to 30 keV/Q) and simultaneously measures their total energy with two low-noise solid state detectors. Solar wind Fe charge state measurements from three time periods of high speed solar wind occurring during a post-shock flow and a coronal hole-associated high speed stream are presented. Analysis of the post-shock flow solar wind indicates the charge state distributions for Fe were peaked at approx +16, indicative of an unusually high coronal temperature (3,000,000 K). In contrast, the Fe charge state distribution observed in a coronal hole-associated high speed stream peaks at approx -9, indicating a much lower coronal temperature (1,400,000 K). This constitutes the first reported measurements of iron charge states in a coronal hole-associated high speed stream.
Document ID
19840005044
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Ipavich, F. M.
(Maryland Univ. College Park, MD, United States)
Galvin, A. B.
(Maryland Univ. College Park, MD, United States)
Gloeckler, G.
(Maryland Univ. College Park, MD, United States)
Hovestadt, D.
(Maryland Univ. College Park, MD, United States)
Klecker, B.
(Maryland Univ. College Park, MD, United States)
Scholer, M.
(Maryland Univ. College Park, MD, United States)
Date Acquired
August 12, 2013
Publication Date
November 1, 1983
Publication Information
Publication: JPL Solar Wind Five
Subject Category
Solar Physics
Accession Number
84N13112
Funding Number(s)
CONTRACT_GRANT: NAS5-26739
CONTRACT_GRANT: BMFT-RV-14-B8/74
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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