Results from Several Persistent Train Spectra Intercompared

Details Results from Several Persistent Train Spectra Intercompared Results from Several Persistent Train Spectra Intercompared

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995em%26p...68..479r&link_type=abstract

Earth, Moon, and Planets, Volume 68, Issue 1-3, pp. 479-486

Computer Science

6

Scientific paper

Some results following from two contemporary photographical programs (Slovakia and Japan) for persistent meteor train spectra are compared. It shows that even though both programs are not too different according to their lenses and films used, the spectral interval detected is very different. In this respect prism as a dispersion element is more favourable than the grating with blaze wavelength near 610 nm. However, some results previously assumed as typicai for presented persistent trains-e.g. the forbidden Herzberg O2 emission, the NO2 continuum and OH red emissions-seem to be substanciated especially due to higher and linear dispersion of those grating spectra.

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