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Evidence for gain on the C VI 182 A transition in a radiation-cooled selenium/Formvar plasmaThin plastic foils coated with selenium have been irradiated using from 4 to 8 beams of the OMEGA laser in a line focus configuration. Spectra were recorded using a 3 meter spectrograph that viewed the plasma along the line focus. Based on a comparison of the intensities of the spectral lines from plasmas with lengths of 1.7, 3.4, 6.8, and 13.6 mm, the C VI n = 3 to 2 transition at 182 A was anomalously intense in the spectra from the longer plasmas. Calculations indicate that the carbon plasma was cooled by radiation from the highly-charged selenium plasma in a time that was smaller than the expansion time of the plasma. These plasma conditions are favorable for the occurrence of population inversions between the n = 2 and 3 levels of C VI resulting from recombination and cascading from higher levels. The measured gain coefficient for the C VI 182 A transition is 3/cm, and this corresponds to a gain-length product of 4 in the longest plasma.
Document ID
19850062803
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Seely, J. F.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Brown, C. M.
(Hulburt (E. O.) Center for Space Research Washington, DC, United States)
Feldman, U.
(U.S. Navy, E. O. Hulburt Center for Space Research, Washington DC, United States)
Richardson, M.
(Rochester, University NY, United States)
Behring, W. E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
July 1, 1985
Publication Information
Publication: Optics Communications
Volume: 54
ISSN: 0030-4018
Subject Category
Lasers And Masers
Accession Number
85A44954
Funding Number(s)
CONTRACT_GRANT: DE-FC08-85DP-40200
CONTRACT_GRANT: DE-AI08-84DP-40092-26
Distribution Limits
Public
Copyright
Other

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