Open AccessRetrieval of stratospheric NO x from 5.3 and 6.2 μm nonlocal thermodynamic equilibrium emissions measured by Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) on Envisat
Author(s) -
Funke B.,
LópezPuertas M.,
von Clarmann T.,
Stiller G. P.,
Fischer H.,
Glatthor N.,
Grabowski U.,
Höpfner M.,
Kellmann S.,
Kiefer M.,
Linden A.,
Mengistu Tsidu G.,
Milz M.,
Steck T.,
Wang D. Y.
Publication year - 2005
Publication title -
journal of geophysical research: atmospheres
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2004jd005225
Subject(s) - stratosphere , atmospheric sounding , michelson interferometer , occultation , environmental science , mixing ratio , atmospheric sciences , depth sounding , physics , thermodynamic equilibrium , atmosphere (unit) , interferometry , remote sensing , astrophysics , meteorology , geology , optics , oceanography , thermodynamics
We present the first global observations of stratospheric NO x (= NO + NO 2 ) from the Michelson Interferometer for Passive Atmospheric Sounding (MIPAS) on Envisat during 24 July, 18 to 27 September, and 11 to 13 October 2002. Volume mixing ratio profiles of both NO x species were derived from MIPAS limb emission spectra by means of an innovative retrieval scheme under consideration of nonlocal thermodynamic equilibrium (non‐LTE) effects. In the quiescent atmosphere, the estimated accuracy of retrieved NO x at the altitude of its stratospheric mixing ratio maximum at 35–40 km is around 1–2 ppbv, and the vertical resolution is around 3.5–6.5 km at altitudes between 20 and 50 km. In order to correctly consider NO 2 non‐LTE effects in the retrievals, the photochemical excitation rate of NO 2 ( v 3 > 0) vibrational states was derived from NO 2 (002→001) emissions and was found to be about 50 times smaller than previously estimated from Limb Infrared Monitor of the Stratosphere (LIMS) measurements. The NO x partitioning of the retrieved data is in excellent agreement with steady state photochemistry, which confirms predicted stratospheric NO( v > 0) non‐LTE population enhancements. The retrieved NO x abundances are also consistent with Halogen Occultation Experiment (HALOE) NO x observations.