Computer Science
Scientific paper
Aug 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009esast.257.....p&link_type=abstract
ESA Scientific Technical Review, vol. 257
Computer Science
Scientific paper
The present report represents the second part of a study on thermodynamic properties of systems important in the space research field. The first part of this study concerned with the calculation of high-temperature thermodynamic properties of Mars-atmosphere components, the second one is about the thermodynamic properties of Jupiter-atmosphere components (H2, H2+, H3+, H+, H-, He, He+, He2+, e-). Also in this case we adopt a two parts division: in the first one, theoretical aspects of the calculation are described focusing our attention on some details, while the second provides tables of spectroscopic data used in the calculation and thermodynamic properties in the temperature range from 50 K to 50000 K at P=1 bar. All results are presented in SI units. Finally, fitting coefficients for nondimensional specific heat are included.
Capitelli Mario
Casavola Alessandro
Colonna G.
Giordano Daniele
Marraffa Lionel
No associations
LandOfFree
Internal partition functions and thermodynamic properties of high-temperature Jupiter-atmosphere species from 50K to 50,000K does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Internal partition functions and thermodynamic properties of high-temperature Jupiter-atmosphere species from 50K to 50,000K, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Internal partition functions and thermodynamic properties of high-temperature Jupiter-atmosphere species from 50K to 50,000K will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-832388