Horizontal thermal structure of the mesosphere from observations of OH/8-3/ band emissions

Details Horizontal thermal structure of the mesosphere from observations of OH/8-3/ band emissions Horizontal thermal structure of the mesosphere from observations of OH/8-3/ band emissions

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981p%26ss...29.1241t&link_type=abstract

Planetary and Space Science, vol. 29, Nov. 1981, p. 1241-1249.

Computer Science

16

Atmospheric Temperature, Hydroxyl Emission, Mesosphere, Spatial Distribution, Temperature Distribution, Airglow, Gravity Waves, Horizontal Orientation, Molecular Rotation, Radiative Lifetime, Spectrophotometry

Scientific paper

Two computerized tilting-filter photometers and a programmable dual axis mirror system have been used to produce maps of OH rotational temperature and intensity. Each map consists of a square array of 121 sky positions. Significant horizontal structure is not generally observed in mesospheric OH(8-3) rotational temperature at Arecibo. However, there is evidence for the occasional occurrence of a thermal wave just after evening twilight.

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