Global observations of nitric oxide in the thermosphere
By C. Barth, K. Mankoff, S. Bailey, S. Solomon. 2003
168 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/b77bff5c6226e95169d74dcebdba15df426b0026
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Citations in the corpus
- Tropospheric tides from 80 to 400 km: Propagation, interannual variability, and solar cycle effects (2009, methodology): “Lower thermospheric nitric oxide densities from the Student Nitric Oxide Explorer (SNOE) [Barth et al., 2003] show a pronounced ‘‘wave-4’’ signature at low latitudes that could be attributed to DE3 density variations [Oberheide and Forbes, 2008b].”
- Energetic Particle Influence on the Earth’s Atmosphere (2015, background): “Their penetration depth is rather small and the energy deposition occurs mainly in the lower thermosphere (above 90 km) and confines to the auroral ovals located over 60–75◦ geomagnetic latitude band (Baker 2000; Barth et al. 2003).”
- Influence of the Precipitating Energetic Particles on Atmospheric Chemistry and Climate (2012, background): “Their energy is mostly deposited in the lower thermosphere (above 90 km) inside the auroral ovals located over the 60 –75 geomagnetic latitude band (Baker et al. 2001; Barth et al. 2003).”
- Simulation of secular trends in the middle atmosphere, 1950–2003 (2007, methodology): “NO is specified using data from the Student Nitric Oxide Explorer (SNOE) satellite [Barth et al., 2003], which has been parameterized as a function of latitude, season, and phase of the solar cycle inMarsh et al.’s [2004] Nitric Oxide Empirical Model (NOEM).”
- Energetic particle precipitation effects on the Southern Hemisphere stratosphere in 1992–2005 (2007, methodology): “These include SH hemispheric auroral and medium energy electron (MEE) power data derived from NOAA POES satellites (http://www.sec.noaa.gov/pmap/PoesSem.html), and thermospheric NO measurements from the Student Nitric Oxide Explorer (SNOE) [Barth et al., 2003].”
- Solar extreme‐ultraviolet irradiance for general circulation models (2005, result): “This is again in better agreement with recent observations [e.g., Russell et al., 1993; Barth et al., 1999; Solomon et al., 1999; Barth et al., 2003; Marsh et al., 2004].”