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Celiberto, R; Armenise, I; Cacciatore, M; Capitelli, M; Esposito, F; Gamallo, P; Janev, R K; Laganà, A; Laporta, V; Laricchiuta, A; Lombardi, A; Rutigliano, M; Sayós, R; Tennyson, J; Wadehra, J M
Plasma sources science & technology, 05/2016, Letnik: 25, Številka: 3Journal Article
The modeling of atmospheric gas, interacting with the space vehicles in re-entry conditions in planetary exploration missions, requires a large set of scattering data for all those elementary processes occurring in the system. A fundamental aspect of re-entry problems is represented by the strong non-equilibrium conditions met in the atmospheric plasma close to the surface of the thermal shield, where numerous interconnected relaxation processes determine the evolution of the gaseous system towards equilibrium conditions. A central role is played by the vibrational exchanges of energy, so that collisional processes involving vibrationally excited molecules assume a particular importance. In the present paper, theoretical calculations of complete sets of vibrationally state-resolved cross sections and rate coefficients are reviewed, focusing on the relevant classes of collisional processes: resonant and non-resonant electron-impact excitation of molecules, atom-diatom and molecule-molecule collisions as well as gas-surface interaction. In particular, collisional processes involving atomic and molecular species, relevant to Earth (N2, O2, NO), Mars (CO2, CO, N2) and Jupiter (H2, He) atmospheres are considered.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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