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Found 7 entries in the Bibliography.
Showing entries from 1 through 7
2009 |
Thermospheric infrared radiance at 4.3 μm is susceptible to the influence of solar-geomagnetic disturbances. Ionization processes followed by ion-neutral chemical reactions lead to vibrationally excited NO+ (i.e., NO+(v)) and subsequent 4.3 μm emission in the ionospheric E-region. Large enhancements of nighttime 4.3 μm emission were observed by the TIMED/SABER instrument during the April 2002 and October\textendashNovember 2003 solar storms. Global measurements of infrared 4.3 μm emission provide an excellent proxy to ... Mertens, Christopher; Winick, Jeremy; Picard, Richard; Evans, David; opez-Puertas, Manuel; Wintersteiner, Peter; Xu, Xiaojing; Mlynczak, Martin; Russell, James; Published by: Advances in Space Research Published on: YEAR: 2009   DOI: 10.1016/j.asr.2008.10.029 |
2004 |
Mertens, CJ; Richards, PG; , Winick; Picard, RH; Paxton, LJ; Wintersteiner, PP; Team, Saber; Published by: Published on: |
The SABER instrument on TIMED continuously measures certain infrared limb radiance profiles with unprecedented sensitivity. Among these are emissions of CO2 ν3 at 4.3 μm, routinely recorded to tangent heights of ~140-150 km, and NO at 5.3 μm, seen to above ~200 km and ~300 km, respectively. We use these infrared channels of SABER and coincident far ultraviolet (FUV) measurements from GUVI on TIMED, to study the geometric storm of April 2002. These all give a consistent measure of auroral energy in ... Winick, Jeremy; Mlynczak, Martin; Wintersteiner, Peter; Martin-Torres, Francisco; Picard, Richard; Paxton, L.; Lopez-Puertas, Manuel; Russell, James; Christensen, Andrew; Gordley, Larry; Published by: Published on: YEAR: 2004   DOI: 10.1117/12.515982 |
2003 |
The Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) experiment on the Thermosphere-Ionosphere Mesosphere Energetics and Dynamics (TIMED) satellite observed the infrared radiative response of the thermosphere to the solar storm events of April 2002. Large radiance enhancements were observed at 5.3 μm, which are due to emission from the vibration-rotation bands of nitric oxide (NO). The emission by NO is indicative of the conversion of solar energy to infrared radiation within the atmosphere and repr ... Mlynczak, Marty; Martin-Torres, F.; Russell, J.; Beaumont, K.; Jacobson, S.; Kozyra, J.; opez-Puertas, M.; Funke, B.; Mertens, C.; Gordley, L.; Picard, R.; Winick, J.; Wintersteiner, P.; Paxton, L.; Published by: Geophysical Research Letters Published on: 03/2003 YEAR: 2003   DOI: 10.1029/2003GL017693 |
, Winick; Mlynczak, MG; Wintersteiner, PP; Martin-Torres, F; Picard, RH; Paxton, L; Lopez-Puertas, M; Mertens, CJ; RUSSELL, JM; Christensen, A; , others; Published by: Published on: |
Winick, J.; Mlynczak, M.; Wintersteiner, P.; Martin-Torres, F.-J.; Picard, R.; Paxton, L.; opez-Puertas, M.; Russell, J.; Christensen, A.; Gordley, L.; Published by: Published on: |
2002 |
, Winick; Wintersteiner, PP; Picard, RH; Paxton, L; opez-Puertas, M; Mlynczak, MG; RUSSELL, JM; Christensen, A; Zhang, Y; Gordley, L; Published by: Published on: |
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