Physics
Scientific paper
Sep 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..707g&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, Sept.-Oct. 1987, p. 707-714. In Russian.
Physics
2
Cloud Cover, Vega Project, Venus Atmosphere, Vertical Distribution, Aerosols, Particle Density (Concentration), Refractivity, Spacecraft Instruments
Scientific paper
Measurements made with the ISAV-A aerosol spectrometers on the Vega 1 and 2 landers are described. The aerosol size distribution is represented by two modes: mode I is described by the Junge distribution from 0.5 to 5 microns, while mode II consists of 2-5-micron particles. Mode II particles are spherical and their refractive index is 1.4 + or - 0.05. Mode II particle concentrations vary sharply at heights from 45 to 50 km, while mode I concentrations vary smoothly at heights from 35 to 55 km, without forming pronounced cloud layers. Submicron aerosol is present at heights of 30-60 km, having a mass density of 0.1-2 mg/cu m for a refractive index of 2.
Ekonomov A. P.
Gnedykh V. I.
Moroz Vasiliy Ivanovich
Moshkin B. E.
Zasova Liudmila V.
No associations
LandOfFree
Vertical structure of the Venus cloud layer over the VEGA 1 and 2 landing sites 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 Vertical structure of the Venus cloud layer over the VEGA 1 and 2 landing sites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Vertical structure of the Venus cloud layer over the VEGA 1 and 2 landing sites will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1676327