Total internal partition sums to support planetary remote sensing
نویسندگان
چکیده
0019-1035/$ see front matter 2011 Elsevier Inc. A doi:10.1016/j.icarus.2011.06.004 ⇑ Corresponding author at: Department of Enviro spheric Sciences, University of Massachusetts Lowell, E-mail address: [email protected] (R.R. G 1 Present address: California Institute of Technology vard, Pasadena, CA 91125, USA. Total internal partition sums are determined from 65 to 3010 K for CO2, COO, CH3D, CH3D, HCCD, CCH6, CH3Br, CH3Br, CF4, HCCCCH, HCCCN, HCCCN, HCCCN, HCCCN, HCCCN, DCCCN, NCCN, NCCN, CS, CS, CS, CS, H2, HD, SO, SO, SO, C3H4, CH3, CS2, SCS, CS2, and SCS. 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. 2011 Elsevier Inc. All rights reserved.
منابع مشابه
Pii: S0022-4073(01)00234-5
Total internal partition sums (TIPS) are calculated for several molecules, which are abundant in non9 terrestrial planetary atmospheres. For all molecules, calculations are performed for the most abundant isotopic species. Partition sums for lesser abundant isotopomers of several molecules are determined as well. The 11 calculations are made for temperatures between 70 and 300 K. The resulting ...
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