Water vapor in the lower atmosphere of Venus: a new analysis of optical spectra measured by entry probes.

Details Water vapor in the lower atmosphere of Venus: a new analysis of optical spectra measured by entry probes. Water vapor in the lower atmosphere of Venus: a new analysis of optical spectra measured by entry probes.

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997kosis..35....3i&link_type=abstract

Kosmicheskie Issledovaniia, Tom 35, No. 1, p. 3 - 17

Computer Science

Databases

2

Venus Atmosphere: Water Vapor

Scientific paper

The authors reanalyze Venera 11, 13, and 14 data using recently available spectroscopic databases with the line-by-line procedure to calculate gaseous opacity and a discrete ordinates radiative transfer program to generate monochromatic intensity spectra. Contrary to the previous interpretation of the same data, mixing ratio was found to be nearly constant and equal to 30±10 ppm in the altitude range of 5 - 60 km. It seems likely that H2O mixing ratio is varying slightly from 40 ppm in the clouds down to the minimum of 20 ppm at 10 - 20 km, although another possibility of constant 30 ppm profile also cannot be rejected. Both models are in good agreement with Earth-based observations within experimental errors of both datasets.

Affiliated with

Also associated with

No associations

Rating

Water vapor in the lower atmosphere of Venus: a new analysis of optical spectra measured by entry probes. 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 Water vapor in the lower atmosphere of Venus: a new analysis of optical spectra measured by entry probes., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Water vapor in the lower atmosphere of Venus: a new analysis of optical spectra measured by entry probes. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1605314