Characteristics of meteors and their ionization trails

Details Characteristics of meteors and their ionization trails Characteristics of meteors and their ionization trails

Feb 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977avest..10..144b&link_type=abstract

(Astronomicheskii Vestnik, vol. 10, July-Sept. 1976, p. 144-150.) Solar System Research, vol. 10, no. 3, Feb. 1977, p. 115-120.

Astronomy and Astrophysics

Astronomy

Atmospheric Ionization, Meteor Trails, Meteoroids, Electron Density (Concentration), Graphs (Charts), Particle Mass, Vertical Distribution

Scientific paper

The characteristics of the ionized trains of meteoric bodies of various density were studied on the basis of radar observations carried out at four points spaced 6 to 8 km apart. The theoretical lengths of ionized trains of meteoric particles with masses ranging between one thousandth and one hundredth of a gram were more than twice the measured lengths. The length of the descending branch of the ionization curve was 0.3 to 0.6 H, where H is the homogeneous height of the atmosphere.

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