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Solar wind iron charge states as ide...
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Lepri, Susan Therese.
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Solar wind iron charge states as identifiers of coronal mass ejections and the characterization of a new low energy particle detector.
Record Type:
Electronic resources : Monograph/item
Title/Author:
Solar wind iron charge states as identifiers of coronal mass ejections and the characterization of a new low energy particle detector./
Author:
Lepri, Susan Therese.
Description:
173 p.
Notes:
Source: Dissertation Abstracts International, Volume: 65-02, Section: B, page: 0789.
Contained By:
Dissertation Abstracts International65-02B.
Subject:
Physics, Astronomy and Astrophysics. -
Online resource:
http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3121984
ISBN:
0496693350
Solar wind iron charge states as identifiers of coronal mass ejections and the characterization of a new low energy particle detector.
Lepri, Susan Therese.
Solar wind iron charge states as identifiers of coronal mass ejections and the characterization of a new low energy particle detector.
- 173 p.
Source: Dissertation Abstracts International, Volume: 65-02, Section: B, page: 0789.
Thesis (Ph.D.)--University of Michigan, 2004.
We examine Fe charge state distributions in the solar wind. The ionic composition of the solar wind directly reflects corona conditions within 4--5 solar radii. Charge state information can be used to determine coronal electron temperatures of s
ISBN: 0496693350Subjects--Topical Terms:
1019521
Physics, Astronomy and Astrophysics.
Solar wind iron charge states as identifiers of coronal mass ejections and the characterization of a new low energy particle detector.
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Solar wind iron charge states as identifiers of coronal mass ejections and the characterization of a new low energy particle detector.
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173 p.
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Source: Dissertation Abstracts International, Volume: 65-02, Section: B, page: 0789.
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Chair: Thomas H. Zurbuchen.
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Thesis (Ph.D.)--University of Michigan, 2004.
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We examine Fe charge state distributions in the solar wind. The ionic composition of the solar wind directly reflects corona conditions within 4--5 solar radii. Charge state information can be used to determine coronal electron temperatures of s
520
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In addition, we also characterize a new delta-doped charge-coupled device (CCD). The new delta-doped CCD has a dead layer that is ∼1/10 th the thickness of previous SSDs used in ACE/SWIGS. Using this detector, we are able to detect H+ and N+
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http://pqdd.sinica.edu.tw/twdaoapp/servlet/advanced?query=3121984
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