http://www.cnr.it/ontology/cnr/individuo/prodotto/ID34643
Molecular physics and kinetics of high-temperature planetary atmospheres (Articolo in rivista)
- Type
- Label
- Molecular physics and kinetics of high-temperature planetary atmospheres (Articolo in rivista) (literal)
- Anno
- 2011-01-01T00:00:00+01:00 (literal)
- Alternative label
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
- M.Capitelli; D.Bruno; G.Colonna; G.DAmmando; F. Esposito; A.Laricchiuta; L.D. Pietanza (literal)
- Pagina inizio
- Pagina fine
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
- Rivista
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroFascicolo
- Note
- ISI Web of Science (WOS) (literal)
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
- Dipartimento di Chimica-Università degli Studi di Bari (Italia);
IMIP-CNR Bari (Italia) (literal)
- Titolo
- Molecular physics and kinetics of high-temperature planetary atmospheres (literal)
- Abstract
- The space exploration is nowadays assisted by realistic
modeling of re-entry conditions of space vehicles in
planetary atmospheres, for design of thermal protection systems.
The detailed kinetic modeling relies on the accurate
description of elementary process dynamics, including the
role of the excitation of the internal degrees of freedom of
chemical species. Efforts in the construction of a complete
and consistent dynamical information are presented, focusing
on hydrogen plasmas relevant to the Jupiter atmosphere.
Examples of numerical experiments are given, emphasizing
the relevance of the adopted state-to-state approach in
reproducing the onset of non-equilibrium internal distributions
governing the plasma-system evolution. (literal)
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