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Record W4232946191 · doi:10.5194/acpd-8-2513-2008

Validation of ozone measurements from the Atmospheric Chemistry Experiment (ACE)

2008· preprint· en· W4232946191 on OpenAlexafffund
É. Dupuy, Kaley A. Walker, Jayanta Kar, C. D. Boone, C. T. McElroy, P. F. Bernath, J. R. Drummond, R. Skelton, Sean D. McLeod, Ryan Hughes, Caroline R. Nowlan, Denis Dufour, J. Zou, F. Nichitiu, Kimberly Strong, Philippe Baron, R. M. Bevilacqua, Thomas Blumenstock, G. E. Bodeker, Tobias Borsdorff, Adam Bourassa, H. Bovensmann, Ian Boyd, Astrid Bracher, Colette Brogniez, John P. Burrows, Valéry Catoire, Simone Ceccherini, Simon Chabrillat, T. Christensen, M. T. Coffey, Ugo Cortesi, J. Davies, C. De Clercq, D. A. Degenstein, Martine De Mazière, P. Démoulin, J. Dodion, B. Firanski, H. Fischer, G. Forbes, L. Froidevaux, D. Fussen, Pierre Gérard, S. Godin-Beekman, F. Goutail, J. Granville, David Griffith, C. S. Haley, James W. Hannigan, M. Höpfner, J. J. Jin, A. Jones, Nicholas Jones, K. W. Jucks, A. Kagawa, Yasuko Kasai, Tobias Kerzenmacher, A. Kleinböhl, Andrew Klekociuk, I. Krämer, H. Küllmann, J. Kuttippurath, E. Kyrölä, Jean‐Christopher Lambert, N. J. Livesey, E. J. Llewellyn, Nicholas Lloyd, Emmanuel Mahieu, G. L. Manney, B. T. Marshall, J. C. McConnell, M. P. McCormick, I. S. McDermid, M. J. McHugh, C. A. McLinden, J. Mellqvist, K. Mizutani, Yasuhiro Murayama, D. Murtagh, H. Oelhaf, A. Parrish, S. V. Petelina, C. Piccolo, Jean‐Pierre Pommereau, C. E. Randall, C. Robert, Chris Roth, Matthias Schneider, C. Senten, T. Steck, A. Strandberg, K. B. Strawbridge, Ralf Sussmann, D. P. J. Swart, D. W. Tarasick, Jeffrey R. Taylor, C. Tétard, L. W. Thomason, Anne M. Thompson, Matthew B. Tully, J. Urban, F. Vanhellemont, T. von Clarmann, Peter von der Gathen, Christian von Savigny, J. W. Waters, J. C. Witte, Mareile Wolff, J. M. Zawodny

Bibliographic record

Venuenot available
Typepreprint
Languageen
FieldEarth and Planetary Sciences
TopicAtmospheric Ozone and Climate
Canadian institutionsYork UniversityUniversity of SaskatchewanUniversity of TorontoDalhousie UniversityEnvironment and Climate Change CanadaUniversity of Waterloo
FundersNatural Sciences and Engineering Research Council of CanadaCanadian Foundation for Climate and Atmospheric SciencesNational Aeronautics and Space AdministrationCalifornia Institute of TechnologyCanadian Space AgencyJet Propulsion LaboratoryUniversity of Toronto
KeywordsSunriseOccultationTroposphereOzoneSunsetStratosphereAtmospheric sciencesEnvironmental scienceAtmospheric chemistryAltitude (triangle)SatelliteMeteorologyRemote sensingPhysicsGeologyAstronomy

Abstract

fetched live from OpenAlex

Abstract. This paper presents extensive validation analyses of ozone observations from the Atmospheric Chemistry Experiment (ACE) satellite instruments: the ACE Fourier Transform Spectrometer (ACE-FTS) and the Measurement of Aerosol Extinction in the Stratosphere and Troposphere Retrieved by Occultation (ACE-MAESTRO) instrument. The ACE satellite instruments operate in the mid-infrared and ultraviolet-visible-near-infrared spectral regions using the solar occultation technique. In order to continue the long-standing record of solar occultation measurements from space, a detailed quality assessment is required to evaluate the ACE data and validate their use for scientific purposes. Here we compare the latest ozone data products from ACE-FTS and ACE-MAESTRO with coincident observations from satellite-borne, airborne, balloon-borne and ground-based instruments, by analysing volume mixing ratio profiles and partial column densities. The ACE-FTS version 2.2 Ozone Update product reports more ozone than most correlative measurements from the upper troposphere to the lower mesosphere. At altitude levels from 16 to 44 km, the mean differences range generally between 0 and +10% with a slight but systematic positive bias (typically +5%). At higher altitudes (45–60 km), the ACE-FTS ozone amounts are significantly larger than those of the comparison instruments by up to ~40% (typically +20%). For the ACE-MAESTRO version 1.2 ozone data product, agreement within ±10% (generally better than ±5%) is found between 18 and 40 km for the sunrise and sunset measurements. At higher altitudes (45–55 km), systematic biases of opposite sign are found between the ACE-MAESTRO sunrise and sunset observations. While ozone amounts derived from the ACE-MAESTRO sunrise occultation data are often smaller than the coincident observations (by as much as −10%), the sunset occultation profiles for ACE-MAESTRO show results that are qualitatively similar to ACE-FTS and indicate a large positive bias (+10 to +30%) in this altitude range. In contrast, there is no significant difference in bias found for the ACE-FTS sunrise and sunset measurements. These systematic effects in the ozone profiles retrieved from the measurements of ACE-FTS and ACE-MAESTRO are being investigated. This work shows that the ACE instruments provide reliable, high quality measurements from the tropopause to the upper stratosphere and can be used with confidence in this vertical domain.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.003
metaresearch head score (Gemma)0.003
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.012
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.003
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.038
GPT teacher head0.238
Teacher spread0.200 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designSimulation or modeling
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations5
Published2008
Admission routes2
Has abstractyes

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