Journal
JOURNAL OF PHYSICS B-ATOMIC MOLECULAR AND OPTICAL PHYSICS
Volume 45, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0953-4075/45/1/015201
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Funding
- Cassini UVIS
- University of Colorado
- NSF [AGS-0938223]
- NASA
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Photodissociation cross sections and oscillator strengths for H-2 from the X-1 Sigma(+)(g) (v(i), J(i)) levels to the continuum levels of the B-1 Sigma(+)(u), C-1 Pi(u), B ''(B) over bar (1)Sigma(+)(u), D' (1) Pi(u) and 5p sigma (1) Sigma(+)(u) states have been calculated. The (v(i), J(i)) state-specific electron impact dissociation cross sections to the continuum levels of these states have been obtained for the first time over a wide energy range using calculated continuum oscillator strengths along with previously published excitation functions of the Lyman and Werner bands. Estimated cross sections to the higher (n >= 5) np sigma (1) Sigma(+)(u) and np pi (1) Pi(u) continua are also provided. Both photon and electron impact excitation cross sections show strong dependences on the initial (v(i), J(i)) quantum numbers. Thermally averaged electron impact cross sections of all singlet ungerade states increase monotonically with temperature. While excitation to the B' (1) Sigma(+)(u) continuum is the dominant dissociation channel at room temperature, the C-1 Pi(u) and B (1) Sigma(+)(u) continua become more important at high temperature (>5000 K). This work, along with the previous calculation of the B' (1)Sigma(+)(u) and D-1 Pi(u) states by Liu et al (2009a J. Phys. B: At. Mol. Opt. Phys. 42 185203), provides the complete electron impact dissociation cross section of H-2 through the singlet ungerade continua. Electron dissociation cross sections of the singlet ungerade continua are provided for the purpose of modelling atmospheric heating, analysis of occultation measurements and the hot atomic hydrogen plume observed at Saturn.
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