2026-09-18T19:06:17Zhttps://dspace.mit.edu/server/oai/requestoai:dspace.mit.edu:1721.1/515782022-01-13T07:54:41Zcom_1721.1_7582com_1721.1_7581col_1721.1_131024
David P. Huenemoerder.
Kesich, Anthony
Massachusetts Institute of Technology. Dept. of Physics.
Massachusetts Institute of Technology. Department of Physics
2010-02-09T16:47:13Z
2010-02-09T16:47:13Z
2009
2009
http://hdl.handle.net/1721.1/51578
491293825
Thesis (S.B.)--Massachusetts Institute of Technology, Dept. of Physics, 2009.
Includes bibliographical references (p. 14-15).
We develop method to extract elemental abundance ratios using temperature-insensitive ratios of x-ray line fluxes for a collisionally ionized plasma. This method is then refined using more realistic plasma models for coronae of active stars. We finally apply the method to multiple sources and compare the results to those obtained via Emission Measure Modeling.
by Anthony Kesich.
S.B.
15 p.
eng
Massachusetts Institute of Technology
M.I.T. theses are protected by
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http://dspace.mit.edu/handle/1721.1/7582
Physics.
Temperature-insensitive line ratios
Thesis
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Publication
unknown
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