A multi-channel spectrometer for airglow observations

Details A multi-channel spectrometer for airglow observations A multi-channel spectrometer for airglow observations

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988p%26ss...36.1269w&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 36, Nov. 1988, p. 1269-1273, 1275-1283. Research supported by SERC.

Computer Science

Performance

1

Airglow, Hydroxyl Emission, Molecular Spectra, Spectral Bands, Upper Atmosphere, Gravity Waves, Internal Waves, Light Scattering, Wave Propagation

Scientific paper

An account is given of the design, construction, and performance of a six-channel spectrometer using tilting interference filters. Spectra of resolution of approximately 2 nm and extending over a range of about 15 nm are obtained once every 2 min at each of six wavelength regions in the visible and near infrared, and are recorded digitally for subsequent analysis. Examples are given of data obtained between 1981 and 1984 showing how the variation of intensities of atomic and molecular emissions and of the temperature deduced from the OH bands can be displayed.

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