Heights of superschmidt meteors and the characteristics of the meteoroids which give rise to them

Details Heights of superschmidt meteors and the characteristics of the meteoroids which give rise to them Heights of superschmidt meteors and the characteristics of the meteoroids which give rise to them

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..19..251l&link_type=abstract

(Astronomicheskii Vestnik, vol. 19, July-Sept. 1985, p. 251-255) Solar System Research (ISSN 0038-0946), vol. 19, no. 3, Jan. 19

Astronomy and Astrophysics

Astronomy

1

Fragmentation, Meteoroids, Stony Meteorites, Atmospheric Density, Height

Scientific paper

It is shown that the observed heights at which faint photographic
meteors disappear are in good agreement with the hypothesis of
quasi-continuous fragmentation of dense stony meteoroids. However, they
are inconsistent with hypotheses with very loose meteroids or dense
stony meteroids which do not fragment.

Affiliated with

Also associated with

No associations

Rating

Heights of superschmidt meteors and the characteristics of the meteoroids which give rise to them 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 Heights of superschmidt meteors and the characteristics of the meteoroids which give rise to them, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Heights of superschmidt meteors and the characteristics of the meteoroids which give rise to them will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1844906