LIMITS ON THE EMISSION FROM FE VIII-XII IN THE HOT LOCAL INTERSTELLAR MEDIUM.

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The majority of the emitted power from an optically thin million degree plasma (such as the one thought to produce the soft xray background) originates in the EUV band at wavelengths longer than 170 degrees A. Lines from Fe VIII - Fe XII dominate the emission in this wavelength region. This paper describes work in progress on the analysis of three years of data from the ALEXIS mission in search of this flux.

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6 p.

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Bloch, J. J. (Jeffrey J.); Roussel-Dupre, D. (Diane); Theiler, J. P. (James P.) & Johnson, E. M. (Elsa M.) January 1, 2001.

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Description

The majority of the emitted power from an optically thin million degree plasma (such as the one thought to produce the soft xray background) originates in the EUV band at wavelengths longer than 170 degrees A. Lines from Fe VIII - Fe XII dominate the emission in this wavelength region. This paper describes work in progress on the analysis of three years of data from the ALEXIS mission in search of this flux.

Physical Description

6 p.

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  • Submitted to: Proceedings of the Conference, "Continuing the Challenge of EUV Astronomy: Current Analysis and Prospects for the Future", held 22-24, July 2001, Jenner, CA, USA

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  • Report No.: LA-UR-01-6369
  • Grant Number: none
  • Office of Scientific & Technical Information Report Number: 975869
  • Archival Resource Key: ark:/67531/metadc929155

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  • January 1, 2001

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  • Nov. 13, 2016, 7:26 p.m.

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  • Dec. 12, 2016, 12:17 p.m.

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Bloch, J. J. (Jeffrey J.); Roussel-Dupre, D. (Diane); Theiler, J. P. (James P.) & Johnson, E. M. (Elsa M.). LIMITS ON THE EMISSION FROM FE VIII-XII IN THE HOT LOCAL INTERSTELLAR MEDIUM., article, January 1, 2001; United States. (digital.library.unt.edu/ark:/67531/metadc929155/: accessed July 18, 2018), University of North Texas Libraries, Digital Library, digital.library.unt.edu; crediting UNT Libraries Government Documents Department.