The atmospheric limb sounders, ACE-FTS on the SCISAT satellite, MIPAS on ESA's Envisat satellite, and MLS on NASA's Aura satellite, take measurements used to retrieve atmospheric profiles of O-3, N2O, H2O, HNO3, and CO. Each was taking measurements between February 2004 and April 2012 (ACE-FTS and MLS are currently operational), providing hundreds of profile coincidences in the Northern and Southern hemispheres, and during local morning and evening. Focusing on determining diurnal and hemispheric biases in the ACE-FTS data, this study compares ACE-FTS version 3.5 profiles that are collocated with MIPAS and MLS, and analyzes the differences between instrument retrievals for Northern and Southern hemispheres and for local morning and evening data. For O-3, ACE-FTS is typically within 5% of mid-stratospheric MIPAS and MLS data and exhibits a positive bias of similar to 10 to 20% in the upper stratosphere - lower mesosphere. For H2O, ACEFTS exhibits an average bias of 5% between 20 and 60 km. For N2O, ACE-FTS agrees with MIPAS and MLS within 20 to +10% up to 45 km and 35 km, respectively. For HNO3, ACEFTS typically agrees within +/- 10% below 30 km, and exhibits a positive bias of similar to 10 to 20% above 30 km. With respect to MIPAS CO, ACE-FTS exhibits an average - 11% bias between 28 and 50 km, and at higher altitudes a positive bias on the order of 10% ( > 100%) in the winter (summer). With respect to winter MLS CO, ACE-FTS is typically within 10% between 25 and 40 km, and has an average bias of - 11% above 40 km. (C) 2016 Elsevier Ltd. All rights reserved:

ACE-FTS ozone, water vapour, nitrous oxide, nitric acid, and carbon monoxide profile comparisons with MIPAS and MLS

Raspollini Piera;
2017

Abstract

The atmospheric limb sounders, ACE-FTS on the SCISAT satellite, MIPAS on ESA's Envisat satellite, and MLS on NASA's Aura satellite, take measurements used to retrieve atmospheric profiles of O-3, N2O, H2O, HNO3, and CO. Each was taking measurements between February 2004 and April 2012 (ACE-FTS and MLS are currently operational), providing hundreds of profile coincidences in the Northern and Southern hemispheres, and during local morning and evening. Focusing on determining diurnal and hemispheric biases in the ACE-FTS data, this study compares ACE-FTS version 3.5 profiles that are collocated with MIPAS and MLS, and analyzes the differences between instrument retrievals for Northern and Southern hemispheres and for local morning and evening data. For O-3, ACE-FTS is typically within 5% of mid-stratospheric MIPAS and MLS data and exhibits a positive bias of similar to 10 to 20% in the upper stratosphere - lower mesosphere. For H2O, ACEFTS exhibits an average bias of 5% between 20 and 60 km. For N2O, ACE-FTS agrees with MIPAS and MLS within 20 to +10% up to 45 km and 35 km, respectively. For HNO3, ACEFTS typically agrees within +/- 10% below 30 km, and exhibits a positive bias of similar to 10 to 20% above 30 km. With respect to MIPAS CO, ACE-FTS exhibits an average - 11% bias between 28 and 50 km, and at higher altitudes a positive bias on the order of 10% ( > 100%) in the winter (summer). With respect to winter MLS CO, ACE-FTS is typically within 10% between 25 and 40 km, and has an average bias of - 11% above 40 km. (C) 2016 Elsevier Ltd. All rights reserved:
2017
Istituto di Fisica Applicata - IFAC
MIPAS
MLS
Profile comparison
Stratospheric and mesospheric trace gases
Satellite limb sounding
ACE-FTS
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/336881
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