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Fuller-Rowell 1993
Fuller-Rowell, T.J. (1993). Modeling the solar cycle change in nitric oxide in the thermosphere and upper mesosphere. Journal of Geophysical Research 98: doi: 10.1029/92JA02201. issn: 0148-0227.

Measurements from the Solar Mesosphere Explorer (SME) satellite have shown that low-latitude nitric oxide densities at 110 km decrease by about a factor of 8 from January 1982 to April 1985. This time period corresponds to the descending phase of the last cycle where the monthly smoothed sunspot number decreased from more than 150 to 1ess than 25. In addition, nitric oxide was observed to vary by a factor of 2 over a solar rotation, during high solar activity. A one-dimensional, globally averaged model of the thermosphere and upper mesosphere has been used to study the height distribution of nitric oxide (NO) and its response to changes in the solar extreme ultraviolet radiation (EUV) through the solar cycle and over a solar rotation. The reference spectra for EUV have been extended, to wavelength down to 0.1 nm, to include all radiation likely to affect the region above 70 km altitude, the lower boundary of the model. The primary source of nitric oxide is the reaction of excited atomic nitrogen, N(2D), with molecular oxygen. The atomic nitrogen is created by a number of ion-neutral reactions and by direct dissociation of molecular nitrogen by photons and photoelectrons. The occurrence of the peak nitric oxide density at or below 115 km is a direct consequence of ionization and dissociation of molecular nitrogen by photoelectrons, which are produced by the solar flux below 30.0 nm (XUV).

Nitric oxide is shown to vary over the solar cycle by a factor of 7 at low latitudes in the lower thermosphere E region, due to the estimated change in the solar EUV flux, in good agreement with the SME satellite observations. The NO density is shown to be strongly dependent on the temperature profile in the lower thermosphere and accounts for the difference between the current model and previous work. Wavelengths less than 1.8 nm have little impact on the NO profile. A factor of 3 change in solar flux below 5.0 nm at high solar activity produced a factor of 2 change in the peak NO density, consistent with SME observations over a solar rotation; this change also lowered the peak to 100 km, consistent with rocket data. ¿American Geophysical Union 1993

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Keywords
Atmospheric Composition and Structure, Thermosphere—composition and chemistry
Journal
Journal of Geophysical Research
http://www.agu.org/journals/jb/
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American Geophysical Union
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