Spectrum of energetic photoelectrons in the Martian and Venusian atmospheres

Details Spectrum of energetic photoelectrons in the Martian and Venusian atmospheres Spectrum of energetic photoelectrons in the Martian and Venusian atmospheres

Nov 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978kosis..16..919a&link_type=abstract

Kosmicheskie Issledovaniia, vol. 16, Nov.-Dec. 1978, p. 919-923. In Russian.

Computer Science

Auger Spectroscopy, Carbon Dioxide, High Energy Electrons, Mars Atmosphere, Photoelectron Spectroscopy, Venus Atmosphere, Electronic Spectra, Energy Bands, Ionization Cross Sections, Photoionization, Spectral Energy Distribution

Scientific paper

The present analysis deals with the production of photoelectrons through ionization of solar radiation at 80 A in the Martian and Venusian upper atmospheres. It is shown that allowance for Auger processes in the CO2 molecule leads to considerable changes in the photoelectron spectrum as compared to calculations without allowance for these processes. Results of calculations of electron fluxes under conditions of local equilibrium are examined.

Affiliated with

Also associated with

No associations

Rating

Spectrum of energetic photoelectrons in the Martian and Venusian atmospheres does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectrum of energetic photoelectrons in the Martian and Venusian atmospheres, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectrum of energetic photoelectrons in the Martian and Venusian atmospheres will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1067661