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Solar wind iron charge states as ide...

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.

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Solar wind iron charge states as identifiers of coronal mass ejections and the characterization of a new low energy particle detector./
作者:	Lepri, Susan Therese.
面頁冊數:	173 p.
附註:	Source: Dissertation Abstracts International, Volume: 65-02, Section: B, page: 0789.
Contained By:	Dissertation Abstracts International65-02B.
標題:	Physics, Astronomy and Astrophysics. -
電子資源:	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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245 1 0 $a 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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500 $a Source: Dissertation Abstracts International, Volume: 65-02, Section: B, page: 0789.
500 $a Chair: Thomas H. Zurbuchen.
502 $a Thesis (Ph.D.)--University of Michigan, 2004.
520 $a 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 $a In addition, we also characterize a new delta-doped charge-coupled device (CCD). The new delta-doped CCD has a dead layer that is &sim;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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790 1 0 $a Zurbuchen, Thomas H., $e advisor
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792 $a 2004
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