Sulfur dioxide and other cloud-related gases as the source of the microwave opacity of the middle atmosphere of Venus

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

9

Microwave Attenuation, Middle Atmosphere, Opacity, Radio Occultation, Sulfur Dioxides, Venus Atmosphere, Absorptivity, Atmospheric Attenuation, Atmospheric Composition, Carbon Dioxide, Gas Chromatography, Venus Probes, Venus, Atmosphere, Opacity, Microwaves, Sulfur Dioxide, Clouds, Models, Absorption, Mariner 10, Pioneer Venus, Comparisons, Carbon Dioxide, Data, Mass Spectrometry, Concentrations, Occultations, Mariner 5, Gases, Water, Gas Chromatography

Scientific paper

Spacecraft radio occultation measurements imply the presence of a nonuniformly mixed gaseous absorber within, but mostly below, the main cloud layer of sulfuric acid-water droplets measured by Pioneer-Venus. Preliminary considerations of the amount, distribution, and effects of sulfur dioxide and other gases, which apparently are associated with and produce the cloud, indicate that they constitute an important, and probably the predominant, source of the observed microwave opacity of the middle atmosphere of Venus.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Sulfur dioxide and other cloud-related gases as the source of the microwave opacity of the middle atmosphere of Venus 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 Sulfur dioxide and other cloud-related gases as the source of the microwave opacity of the middle atmosphere of Venus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sulfur dioxide and other cloud-related gases as the source of the microwave opacity of the middle atmosphere of Venus will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-782660

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.