Physics
Scientific paper
Sep 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20..730a&link_type=abstract
Kosmicheskie Issledovaniia, vol. 20, Sept.-Oct. 1982, p. 730-735. In Russian.
Physics
3
Ablation, Earth Atmosphere, Mars Atmosphere, Meteorite Collisions, Meteoroids, Venus Atmosphere, Approximation, Meteor Trails, Stony Meteorites, Vaporizing
Scientific paper
An investigation is presented of the motion of a meteoroid particle in the rarefied layers of the atmospheres of the earth, Venus, and Mars, with allowance for its nonstationary heating and change in shape due to vaporization. Numerical calculations are performed for a series of stony meteoroid particles, with sizes less than 1 mm for initial entry velocities of 15-60 km/s and entry angles of 10-90 deg. An assessment is made of meteoroid ablation rate and temperature, luminescence intensity, and the electron density of the meteor trail at successive moments of time of the meteor's passage through the atmosphere. For the earth's atmosphere, results are compared with known approximate solutions of the physical theory of meteors and with observational results.
Apshtein E. Z.
Piliugin N. N.
Vartanian N. V.
No associations
LandOfFree
Investigation of meteor ablation in the atmospheres of the earth, Mars, and 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 Investigation of meteor ablation in the atmospheres of the earth, Mars, and Venus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Investigation of meteor ablation in the atmospheres of the earth, Mars, and Venus will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1262080