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Validation of the Aura Microwave Limb Sounder HNO 3 measurements
Author(s) -
Santee M. L.,
Lambert A.,
Read W. G.,
Livesey N. J.,
Cofield R. E.,
Cuddy D. T.,
Daffer W. H.,
Drouin B. J.,
Froidevaux L.,
Fuller R. A.,
Jarnot R. F.,
Knosp B. W.,
Manney G. L.,
Perun V. S.,
Snyder W. V.,
Stek P. C.,
Thurstans R. P.,
Wagner P. A.,
Waters J. W.,
Muscari G.,
de Zafra R. L.,
Dibb J. E.,
Fahey D. W.,
Popp P. J.,
Marcy T. P.,
Jucks K. W.,
Toon G. C.,
Stachnik R. A.,
Bernath P. F.,
Boone C. D.,
Walker K. A.,
Urban J.,
Murtagh D.
Publication year - 2007
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 - 10.1029/2007jd008721
Subject(s) - microwave limb sounder , stratosphere , troposphere , environmental science , remote sensing , altitude (triangle) , advanced microwave sounding unit , satellite , atmospheric sounding , mesosphere , atmospheric sciences , microwave , meteorology , geology , physics , mathematics , geometry , astronomy , quantum mechanics
We assess the quality of the version 2.2 (v2.2) HNO 3 measurements from the Microwave Limb Sounder (MLS) on the Earth Observing System Aura satellite. The MLS HNO 3 product has been greatly improved over that in the previous version (v1.5), with smoother profiles, much more realistic behavior at the lowest retrieval levels, and correction of a high bias caused by an error in one of the spectroscopy files used in v1.5 processing. The v2.2 HNO 3 data are scientifically useful over the range 215 to 3.2 hPa, with single‐profile precision of ∼0.7 ppbv throughout. Vertical resolution is 3–4 km in the upper troposphere and lower stratosphere, degrading to ∼5 km in the middle and upper stratosphere. The impact of various sources of systematic uncertainty has been quantified through a comprehensive set of retrieval simulations. In aggregate, systematic uncertainties are estimated to induce in the v2.2 HNO 3 measurements biases that vary with altitude between ±0.5 and ±2 ppbv and multiplicative errors of ±5–15% throughout the stratosphere, rising to ∼±30% at 215 hPa. Consistent with this uncertainty analysis, comparisons with correlative data sets show that relative to HNO 3 measurements from ground‐based, balloon‐borne, and satellite instruments operating in both the infrared and microwave regions of the spectrum, MLS v2.2 HNO 3 mixing ratios are uniformly low by 10–30% throughout most of the stratosphere. Comparisons with in situ measurements made from the DC‐8 and WB‐57 aircraft in the upper troposphere and lowermost stratosphere indicate that the MLS HNO 3 values are low in this region as well, but are useful for scientific studies (with appropriate averaging).

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