Observations of infrared radiative cooling in the thermosphere on daily to multiyear timescales from the TIMED/SABER instrument

• Published in: Journal of Geophysical Research. A. Space Physics Vol. 115; no. A3
• Main Authors: Mlynczak, Martin G., Hunt, Linda A., Thomas Marshall, B., Martin-Torres, F. Javier, Mertens, Christopher J., Russell III, James M., Remsberg, Ellis E., López-Puertas, Manuel, Picard, Richard, Winick, Jeremy, Wintersteiner, Peter, Thompson, R. Earl, Gordley, Larry L.
• Format: Journal Article
• Language: English
• Published: Washington, DC Blackwell Publishing Ltd 01.03.2010; American Geophysical Union
• Subjects: Atmosfärsvetenskap; Atmosphere; Atmospheric science; Atmospheric sciences; Carbon dioxide; climate; Climate change; Climatic data; Earth; Earth sciences; Earth, ocean, space; Emissions; Exact sciences and technology; Ionosphere; Latitude; Nitric oxide; Polar environments; radiative cooling; thermosphere; Upper atmosphere; atmosphere; Energetics; satellites; carbon dioxide; NASA; Cooling rate; Radiation flux; exhibits; Mesosphere; ionosphere; sounding; Sun; nitrogen oxide; Earth; dynamics; instruments; Nitric oxide; radiometry; Short term variation; cooling; solar cycles; sunspots; Radiated power
• ISSN: 0148-0227; 2169-9380; 2169-9402; 2156-2202; 2169-9402
• DOI: 10.1029/2009JA014713

We present observations of the infrared radiative cooling by carbon dioxide (CO2) and nitric oxide (NO) in Earth's thermosphere. These data have been taken over a period of 7 years by the Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument on the NASA Thermosphere‐Ionosphere‐Mesosphere Energetics and Dynamics (TIMED) satellite and are the dominant radiative cooling mechanisms for the thermosphere. From the SABER observations we derive vertical profiles of radiative cooling rates (W m−3), radiative fluxes (W m−2), and radiated power (W). In the period from January 2002 through January 2009, we observe a large decrease in the cooling rates, fluxes, and power consistent with the declining phase of solar cycle 23. The power radiated by NO during 2008 when the Sun exhibited few sunspots was nearly one order of magnitude smaller than the peak power observed shortly after the mission began. Substantial short‐term variability in the infrared emissions is also observed throughout the entire mission duration. Radiative cooling rates and radiative fluxes from NO exhibit fundamentally different latitude dependence than do those from CO2, with the NO fluxes and cooling rates being largest at high latitudes and polar regions. The cooling rates are shown to be derived relatively independent of the collisional and radiative processes that drive the departure from local thermodynamic equilibrium (LTE) in the CO2 15 μm and the NO 5.3 μm vibration‐rotation bands. The observed NO and CO2 cooling rates have been compiled into a separate data set and represent a climate data record that is available for use in assessments of radiative cooling in upper atmosphere general circulation models.