Validation of NO2 and NO from the Atmospheric Chemistry Experiment (ACE)
Tobias Kerzenmacher
(1)
,
Mareile Wolff
(1)
,
Kimberly Strong
(1)
,
Eric Dupuy
(2)
,
Kaley Walker
(1, 2)
,
Leonard Amekudzi
(3)
,
R.L. Batchelor
(1)
,
P.F. Bernath
(4, 2)
,
Gwenaël Berthet
(5)
,
T. Blumenstock
(6)
,
C.D. Boone
(2)
,
K. Bramstedt
(3)
,
Colette Brogniez
(7)
,
S. Brohede
(8)
,
J.P. Burrows
(3)
,
Valéry Catoire
(5)
,
J. Dodion
(9)
,
J.R. Drummond
(1, 10)
,
D.G. Dufour
(11)
,
B. Funke
(12)
,
D. Fussen
(9)
,
Florence Goutail
(13)
,
D.W. T. Griffith
(14)
,
C.S. Haley
(15)
,
F. Hendrick
(9)
,
Michael Höpfner
(6)
,
Nathalie Huret
(5)
,
N. Jones
(14)
,
J. Kar
(1)
,
I. Kramer
(6)
,
E.J. Llewellyn
(16)
,
M. López-Puertas
(12)
,
G. Manney
(17, 18)
,
C.T. Mcelroy
(19, 1)
,
C.A. Mclinden
(19)
,
S. Melo
(20)
,
S. Mikuteit
(6)
,
D. Murtagh
(8)
,
F. Nichitiu
(1)
,
J. Notholt
(3)
,
C. Nowlan
(1)
,
C. Piccolo
(21)
,
Jean-Pierre Pommereau
(13)
,
C. Randall
(22)
,
P. Raspollini
(23)
,
M. Ridolfi
(24)
,
A. Richter
(3)
,
M. Schneider
(6)
,
O. Schrems
(25)
,
M. Silicani
(20)
,
G.P. Stiller
(6)
,
James Taylor
(1)
,
C. Tétard
(7)
,
M. Toohey
(1)
,
F. Vanhellemont
(9)
,
T. Warneke
(3)
,
J.M. Zawodny
(26)
,
J. Zou
(1)
1
Department of Physics [Toronto]
2 Department of Chemistry [Waterloo]
3 IUP - Institute of Environmental Physics [Bremen]
4 Department of Chemistry [York, UK]
5 LPCE - Laboratoire de physique et chimie de l'environnement
6 IMK-IFU - Institut für Meteorologie und Klimaforschung - Atmosphärische Umweltforschung
7 LOA - Laboratoire d’Optique Atmosphérique - UMR 8518
8 Department of Radio and Space Science [Göteborg]
9 BIRA-IASB - Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique
10 Department of Physics and Atmospheric Science [Halifax]
11 Picomole Instruments Inc.
12 IAA - Instituto de Astrofísica de Andalucía
13 SA - Service d'aéronomie
14 University of Wollongong [Australia]
15 CRESS - Centre for Research in Earth and Space Science [Toronto]
16 ISAS - Institute of Space and Atmospheric Studies [Saskatoon]
17 JPL - Jet Propulsion Laboratory
18 NMT - New Mexico Institute of Mining and Technology [New Mexico Tech]
19 ECCC - Environment and Climate Change Canada
20 CSA - Canadian Space Agency
21 AOPP - Department of Atmospheric, Oceanic and Planetary Physics [Oxford]
22 LASP - Laboratory for Atmospheric and Space Physics [Boulder]
23 IFAC - Istituto di Fisica Applicata "Nello Carrara"
24 Dipartimento di Chimica Fisica ed Inorganica
25 AWI - Alfred-Wegener-Institut, Helmholtz-Zentrum für Polar- und Meeresforschung = Alfred Wegener Institute for Polar and Marine Research = Institut Alfred-Wegener pour la recherche polaire et marine
26 LaRC - NASA Langley Research Center [Hampton]
2 Department of Chemistry [Waterloo]
3 IUP - Institute of Environmental Physics [Bremen]
4 Department of Chemistry [York, UK]
5 LPCE - Laboratoire de physique et chimie de l'environnement
6 IMK-IFU - Institut für Meteorologie und Klimaforschung - Atmosphärische Umweltforschung
7 LOA - Laboratoire d’Optique Atmosphérique - UMR 8518
8 Department of Radio and Space Science [Göteborg]
9 BIRA-IASB - Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique
10 Department of Physics and Atmospheric Science [Halifax]
11 Picomole Instruments Inc.
12 IAA - Instituto de Astrofísica de Andalucía
13 SA - Service d'aéronomie
14 University of Wollongong [Australia]
15 CRESS - Centre for Research in Earth and Space Science [Toronto]
16 ISAS - Institute of Space and Atmospheric Studies [Saskatoon]
17 JPL - Jet Propulsion Laboratory
18 NMT - New Mexico Institute of Mining and Technology [New Mexico Tech]
19 ECCC - Environment and Climate Change Canada
20 CSA - Canadian Space Agency
21 AOPP - Department of Atmospheric, Oceanic and Planetary Physics [Oxford]
22 LASP - Laboratory for Atmospheric and Space Physics [Boulder]
23 IFAC - Istituto di Fisica Applicata "Nello Carrara"
24 Dipartimento di Chimica Fisica ed Inorganica
25 AWI - Alfred-Wegener-Institut, Helmholtz-Zentrum für Polar- und Meeresforschung = Alfred Wegener Institute for Polar and Marine Research = Institut Alfred-Wegener pour la recherche polaire et marine
26 LaRC - NASA Langley Research Center [Hampton]
P.F. Bernath
- Fonction : Auteur
Gwenaël Berthet
- Fonction : Auteur
- PersonId : 18957
- IdHAL : gwenael-berthet
- ORCID : 0000-0003-3169-1636
- IdRef : 070409153
Valéry Catoire
- Fonction : Auteur
- PersonId : 185143
- IdHAL : valery-catoire
- ORCID : 0000-0001-8126-3096
- IdRef : 148082920
Florence Goutail
- Fonction : Auteur
- PersonId : 756445
- ORCID : 0000-0002-1431-1542
Nathalie Huret
- Fonction : Auteur
- PersonId : 1066733
C.T. Mcelroy
- Fonction : Auteur
Jean-Pierre Pommereau
- Fonction : Auteur
- PersonId : 756460
- ORCID : 0000-0002-8285-9526
- IdRef : 068864035
James Taylor
- Fonction : Auteur
- PersonId : 184137
- IdHAL : james-taylor
- ORCID : 0000-0001-9709-8689
Résumé
Vertical profiles of NO2 and NO have been obtained from solar occultation measurements by the Atmospheric Chemistry Experiment (ACE), using an infrared Fourier Transform Spectrometer (ACE-FTS) and (for NO2) an ultraviolet-visible-near-infrared spectrometer, MAESTRO (Measurement of Aerosol Extinction in the Stratosphere and Troposphere Retrieved by Occultation). In this paper, the quality of the ACE-FTS version 2.2 NO2 and NO and the MAESTRO version 1.2 NO2 data are assessed using other solar occultation measurements (HALOE, SAGE II, SAGE III, POAM III, SCIAMACHY), stellar occultation measurements (GOMOS), limb measurements (MIPAS, OSIRIS), nadir measurements (SCIAMACHY), balloon-borne measurements (SPIRALE, SAOZ) and ground-based measurements (UV-VIS, FTIR). Time differences between the comparison measurements were reduced using either a tight coincidence criterion, or where possible, chemical box models. ACE-FTS NO2 and NO and the MAESTRO NO2 are generally consistent with the correlative data. The ACE-FTS and MAESTRO NO2 volume mixing ratio (VMR) profiles agree with the profiles from other satellite data sets to within about 20% between 25 and 40 km, with the exception of MIPAS ESA (for ACE-FTS) and SAGE II (for ACE-FTS (sunrise) and MAESTRO) and suggest a negative bias between 23 and 40 km of about 10%. MAESTRO reports larger VMR values than the ACE-FTS. In comparisons with HALOE, ACE-FTS NO VMRs typically (on average) agree to ±8% from 22 to 64 km and to +10% from 93 to 105 km, with maxima of 21% and 36%, respectively. Partial column comparisons for NO2 show that there is quite good agreement between the ACE instruments and the FTIRs, with a mean difference of +7.3% for ACE-FTS and +12.8% for MAESTRO.
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