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Solar photo rates for planetary atmospheres and atmospheric pollutants
- W. Huebner, J. Keady, S. Lyon
- Physics, Geology
- 1 June 1984
Unattenuated solar photo rate coefficients and excess energies for dissociation, ionization, and dissociative ionization are presented for atomic and molecular species that have been identified or…
Photoionization and photodissociation rates in solar and blackbody radiation fields
- W. Huebner, J. Mukherjee
- Physics, Chemistry
- 1 February 2015
Heat and Gas Diffusion in Comet Nuclei
- W. Huebner, J. Benkhoff, D. Prialnik
- Physics
- 1 June 2006
Synthesis of complex molecules in dense interstellar clouds via gas-phase chemistry: a pseudo time-dependent calculation
- C. Leung, E. Herbst, W. Huebner
- Physics
- 1 October 1984
On presente un modele detaille pour la chimie en phase gazeuse des nuages interstellaires denses qui inclut, pour la premiere fois, des reactions qui produisent et qui detruisent un echantillon…
Cometary gas and plasma flow with detailed chemistry
- H. Schmidt, R. Wegmann, W. Huebner, D. Boice
- Physics
- 1 April 1988
First Polymer in Space Identified in Comet Halley
- W. Huebner
- PhysicsScience
- 7 August 1987
The heavy-ion mass spectrum obtained in the inner coma of comet Halley with the PICCA instrument on the Giotto spacecraft has been examined. Short polymer chains of polyoxymethylene and their decay…
First Halley Multicolour Camera imaging results from Giotto
- H. Keller, C. Arpigny, K. Wilhelm
- Physics
- 15 May 1986
The first imaging results from the Halley Multicolour Camera (HMC) during the Giotto fly-by of comet Halley provide images centred on the brightest part of the inner coma which show the silhouette of…
Molecular equilibrium with condensation. [in astrophysics]
- C. Sharp, W. Huebner
- Physics
- 1 February 1990
Minimization of the Gibbs energy of formation for species of chemical elements and compounds in their gas and condensed phases determines their relative abundances in a mixture in chemical…
Solar photo rate coefficients
- W. Huebner, C. W. Carpenter
- Physics, Chemistry
- 1 October 1979
Photo rate coefficients based on wavelength dependent solar photon flux at 1 AU heliocentric distance have been determined for atomic hydrogen, carbon, nitrogen, and oxygen, and for some molecules…
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