On the very high velosity meteors

Details On the very high velosity meteors On the very high velosity meteors

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.495..557h&link_type=abstract

In: Proceedings of the Meteoroids 2001 Conference, 6 - 10 August 2001, Kiruna, Sweden. Ed.: Barbara Warmbein. ESA SP-495, Noordw

Astronomy and Astrophysics

Astronomy

Meteor, Radar Echo, Velocity, Amor, Hyperbolic Meteors, Interstellar Meteors

Scientific paper

The reexamination of radar methods used in the AMOR meteor project for the determination of meteor velocities leads to the conclusion that the sets of highly hyperbolic velocities in the range 100 - 500 km s-1, based on the time-lag method and its combinations, cannot be accepted, until the approval of this dataset by means of suggested tests of meteor astronomy is not made. Therefore, also the conclusions based on these highly hyperbolic orbits, derived from AMOR system needs some revision.

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