On the heights of maximum brightness of faint photographic meteors.

Details On the heights of maximum brightness of faint photographic meteors. On the heights of maximum brightness of faint photographic meteors.

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994avest..28..107n&link_type=abstract

Astronomicheskii Vestnik, Tom 28, No. 6, p. 107 - 110

Astronomy and Astrophysics

Astronomy

Meteors: Trajectories

Scientific paper

The observed dependence of the average heights of maximum brightness of the super-Schmidt meteors versus its velocity was analysed. On the basis of the physical theory of quasi-continuous fragmentation of meteoroids the theoretical dependence of the heights of the maximum brightness versus its velocity was received. The authors compare observed and theoretical dependences and came to the conclusion that the majority of super-Schmidt meteors is produced by dense meteoroids of ordinary chondrite types (δ≅ 3.5 g/cm3) in the case of slow fragmentation, and carbonaceous chondrites (δ = 1 g/cm3) in the case of fast fragmentation.

Affiliated with

Also associated with

No associations

Rating

On the heights of maximum brightness of faint photographic meteors. 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 On the heights of maximum brightness of faint photographic meteors., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the heights of maximum brightness of faint photographic meteors. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1327247