Laboratory measurements of the solar reemission factor G1.0 of the NO-gamma band at 2147 A for the determination of the density of nitric oxide in the D-region of the ionosphere

Details Laboratory measurements of the solar reemission factor G1.0 of the NO-gamma band at 2147 A for the determination of the density of nitric oxide in the D-region of the ionosphere Laboratory measurements of the solar reemission factor G1.0 of the NO-gamma band at 2147 A for the determination of the density of nitric oxide in the D-region of the ionosphere

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...7931130l&link_type=abstract

"Laboratory measurements of the solar reemission factor g sub 1.0 of the NO-gamma band at 2147 A for the determination of the de

Computer Science

Light Emission, Nitric Oxide, Air Pollution, Anomalies, D Region, Density (Number/Volume), Gamma Rays, Radio Waves, Winter

Scientific paper

The reemission factor of the solar ultraviolet resonance emission in the NO gamma (1.0) band was determined under laboratory conditions in order to calculate the density of nitric oxide in the D region of the ionosphere. A special NO measuring chamber was built for this purpose. The most commonly used valve of 9 = 3.93 x ten to the -6 power by Pearce could not be confirmed by directphoton measurement, but rather the still unpublished valve of 9 = 7.05 x ten to the -6 power by Witt could. Thus, earlier rocket measurements are to be corrected, since different g factors were used. This work is related to the German rocket compaign (1975 to 1977) which investigated the winter anomaly of radio wave absorption in the D layer which is chiefly caused by the ionization of NO.

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