Journal
ICARUS
Volume 215, Issue 1, Pages 391-400Publisher
ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2011.06.004
Keywords
Abundances, Atmospheres; Atmospheres, Composition; Radiative transfer; Spectroscopy
Categories
Funding
- National Science Foundation [ATM-0803135]
- NASA [NNX10AB94G]
- Earth Observing System (EOS) [NAG5-13534]
- Directorate For Geosciences
- Div Atmospheric & Geospace Sciences [803135] Funding Source: National Science Foundation
- NASA [136365, NNX10AB94G] Funding Source: Federal RePORTER
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Total internal partition sums are determined from 65 to 3010 K for (13)C(18)O(2), (13)C(18)O(17)O, (12)CH(3)D, (13)CH(3)D, H(12)C(12)CD, (13)C(12)CH(6), (12)CH(3)(79)Br, (12)CH(3)(81)Br, (12)CF(4), H(12)C(12)C(12)C(12)CH, H(12)C(12)C(12)C(14)N, H(12)C(12)C(13)C(14)N, H(12)C(13)C(12)C(14)N, H(13)C(12)C(12)C(14)N, H(12)C(12)C(12)C(15)N, D(12)C(12)C(12)C(14)N, (14)N(12)C(12)C(14)N, (15)N(12)C(12)C(15)N, (12)C(32)S, (12)C(33)S, (12)C(34)S, (13)C(32)S, H(2), HD, (32)S(16)O, (32)S(18)O, (34)S(16)O, (12)C(3)H(4), (12)CH(3), (12)C(32)S(2), (32)S(12)C(34)S, (13)C(32)S(2), and (32)S(12)C(33)S. These calculations complete the partition sum data needed for additional isotopologues in HITRAN2008 and also extend the partition sums to molecules of astrophysical interest. These data, at 25 K steps, are incorporated into a FORTRAN code (TIPS_2011.for) that can be used to rapidly generate the data at any temperature in the range 70-3000 K. (C) 2011 Elsevier Inc. All rights reserved.
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