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Molecular processes in cometsThe transition dipole moments of the c 3 Pi u - a 3 Sigma g +, i 3 Pi g - c 3 Pi u, and i 3 Pi g - b 3 Sigma u + transitions of molecular hydrogen were calculated over a wide range of internuclear distances R. Calculations of the emission spectra are nearing completion. Substantial progress was made in the calculation of the absorption coefficient of a colliding pair of hydrogen atoms in the binary encounter approximation. Detailed calculations were performed on the continuum emission arising from the excitation of the a 3 sigma g + state of H2 by the impact of electrons of various energies. Each curve is labelled by the electron energy in electron volts. The strong emission near Lyman alpha is interesting in that it is produced by excitation of molecular hydrogen.
Document ID
19890002300
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Dalgarno, A.
(Smithsonian Astrophysical Observatory Cambridge, MA, United States)
Date Acquired
September 5, 2013
Publication Date
September 1, 1988
Subject Category
Astrophysics
Report/Patent Number
NASA-CR-182742
SAPR-21
NAS 1.26:182742
Report Number: NASA-CR-182742
Report Number: SAPR-21
Report Number: NAS 1.26:182742
Accession Number
89N11671
Funding Number(s)
CONTRACT_GRANT: NSG7-421
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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