The Typical Perseid Meteor Spectrum

Details The Typical Perseid Meteor Spectrum The Typical Perseid Meteor Spectrum

Nov 1953

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1953natur.172..853m&link_type=abstract

Nature, Volume 172, Issue 4384, pp. 853-854 (1953).

Physics

2

Scientific paper

THE first Perseid meteor spectrum was photographed by S. Blajko at Moscow on a blue-sensitive plate on August 12, 19041,2; but up to 1934 only two additional examples of such photographs had been secured. The emission lines of Fe I, Ca I, Ca II, Mg I, Mn I and Al I were identified in the early photographic spectra, the H and K lines of Ca II generally being the strongest feature.

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