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Optical constants of organic tholins produced in a simulated Titanian atmosphere - From soft X-ray to microwave frequenciesThe determination of the real (n) and imaginary (k) parts of the complex refractive index of thin films of the dark reddish organic solids called tholins, produced by continuous D.C. discharge through a 0.9 N2/0.1 CH4 gas mixture at 0.2 mb, is reported. For the 250 A-1000 micron wavelength range, n and k have been determined from a combination of transmittance, specular reflectance, interferometric, Brewster angle, and ellipsometric polarization measurements. Experimental uncertainties are estimated at + or -0.05 for n and + or -30 percent for k. The results in the visible range are consistent with deductions made by ground-based and spacecraft observations of Titan, in whose atmosphase tholins are thought to be present.
Document ID
19850030586
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Khare, B. N.
(Cornell Univ. Ithaca, NY, United States)
Sagan, C.
(Cornell University Ithaca, NY, United States)
Arakawa, E. T.
(Cornell Univ. Ithaca, NY, United States)
Suits, F.
(Cornell Univ. Ithaca, NY, United States)
Callcott, A.
(Cornell Univ. Ithaca, NY, United States)
Williams, M. W.
(Oak Ridge National Laboratory Oak Ridge, TN, United States)
Date Acquired
August 12, 2013
Publication Date
October 1, 1984
Publication Information
Publication: Icarus
Volume: 60
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
85A12737
Funding Number(s)
CONTRACT_GRANT: W-7405-ENG-26
CONTRACT_GRANT: NGR-33-010-101
Distribution Limits
Public
Copyright
Other

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