Spectral meteor observations by the method of instantaneous exposure

Details Spectral meteor observations by the method of instantaneous exposure Spectral meteor observations by the method of instantaneous exposure

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980avest..13..243b&link_type=abstract

(Astronomicheskii Vestnik, vol. 13, Oct.-Dec. 1979, p. 243-247.) Solar System Research, vol. 13, no. 4, Apr. 1980, p. 193-197. T

Astronomy and Astrophysics

Astronomy

1

Astronomical Photography, Astronomical Photometry, Line Spectra, Meteoroids, Tables (Data)

Scientific paper

An analysis of a meteor spectrum with dispersion 67 A/mm, photographed with exposures of 0.003 sec, is presented. Spectral line wavelengths are determined to plus or minus 2 A. The Na I doublet lines of Mg I, and 42 various FE I multiplets stand out among the brightest lines. Lines of Ca I, Ni I, Cr I, Mn I, and Co I are identifiable, and the first positive system of molecular nitrogen bands (N2) is visible also. A very weak continuous spectrum is observed in the wavelength region 5898-6900 A.

Affiliated with

Also associated with

No associations

Rating

Spectral meteor observations by the method of instantaneous exposure 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 Spectral meteor observations by the method of instantaneous exposure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral meteor observations by the method of instantaneous exposure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1698024