Analysis of photometric spectra of 17 meteors

Details Analysis of photometric spectra of 17 meteors Analysis of photometric spectra of 17 meteors

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mmsa.reptq....m&link_type=abstract

In its Meteors and Meteor Spectra Anal. 9 p (SEE N83-14040 04-91)

Physics

Meteoritic Composition, Meteoroids, Photometry, Spectroscopic Telescopes, Spectroscopy, Spectrum Analysis, Aquarid Meteoroids, Celestial Bodies, Geminid Meteoroids, Halley'S Comet, Meteoroid Showers, Orionid Meteoroids

Scientific paper

The initial phase of the photometry which involved 17 meteor spectra consisting of eight Geminid spectra, six Orionid spectra and three Eta Aquarid spectra is discussed. Among these 17 spectra it is found that the Geminid spectra are of the best quality and are used for the identification of the atomic lines and molecular bands that normally appear on video tape spectra. The data from the Geminid records are used for developing calibration techniques in photometry. The Orionid and Eta Aquarid spectra are chosen for early analysis because of the current interest in all physical and chemical data relating to Comet Halley.

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