Ionization, dissociation, and heating efficiencies of cosmic rays in a gas of molecular hydrogen

Details Ionization, dissociation, and heating efficiencies of cosmic rays in a gas of molecular hydrogen Ionization, dissociation, and heating efficiencies of cosmic rays in a gas of molecular hydrogen

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...219..750c&link_type=abstract

Astrophysical Journal, Part 1, vol. 219, Jan. 15, 1978, p. 750-752.

Astronomy and Astrophysics

Astrophysics

57

Cosmic Rays, Gas Dissociation, Gas Heating, Gas Ionization, Hydrogen Clouds, Interstellar Gas, Energy Conversion Efficiency, Gas-Ion Interactions, Hydrogen Atoms, Hydrogen Ions

Scientific paper

Calculations are presented for the efficiencies with which cosmic rays (having energies of 1-100 MeV) traversing a molecular hydrogen gas produce H2(+), H(+), and H(-) ions, and H atoms. More specifically, detailed descriptions are made of both the primary and secondary processes of such rays, noting parameters including proton impact ionization cross sections and mean energies of secondary electrons.

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