Venera 13 and 14 - Mass spectroscopy of the atmosphere

Details Venera 13 and 14 - Mass spectroscopy of the atmosphere Venera 13 and 14 - Mass spectroscopy of the atmosphere

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983kosis..21..410i&link_type=abstract

Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 21, May-June 1983, p. 410-420. In Russian.

Computer Science

Atmospheric Composition, Mass Spectroscopy, Venera Satellites, Venus Atmosphere, Argon Isotopes, Krypton Isotopes, Neon Isotopes, Nitrogen Isotopes, Xenon Isotopes

Scientific paper

RF mass spectrometers on the Venera 13 and 14 probes were used to study the composition of neon, argon, krypton, xenon, nitrogen, and carbon isotopes in the Venus atmosphere. A comparison of mass spectra indicates that the argon isotope composition in the Venus atmosphere is anomalous: the peaks of Ar-40 and Ar-36 are roughly equal, while their proportion is 300:1 for terrestrial argon. An attempt is made to explain the discrepancy between the present data on Ar-36 and the Pioneer-Venus data.

Affiliated with

Also associated with

No associations

Rating

Venera 13 and 14 - Mass spectroscopy of the atmosphere 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 Venera 13 and 14 - Mass spectroscopy of the atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Venera 13 and 14 - Mass spectroscopy of the atmosphere will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1586828