On the consistency of HNO3 and NO2 in the Aleutian High region from the Nimbus 7 LIMS Version 6 data set

This study uses photochemical calculations along kinematic trajectories in conjunction with Limb Infrared Monitor of the Stratosphere (LIMS) observations to examine the changes in HNO 3 and NO 2 near 30 hPa in the region of the Aleutian High (AH) during the minor warming event of January 1979. An ea...

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Published in:Atmospheric Measurement Techniques
Main Authors: Remsberg, Ellis, Natarajan, Murali, Harvey, V. Lynn
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/amt-11-3611-2018
https://amt.copernicus.org/articles/11/3611/2018/
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spelling ftcopernicus:oai:publications.copernicus.org:amt64746 2023-05-15T17:40:01+02:00 On the consistency of HNO3 and NO2 in the Aleutian High region from the Nimbus 7 LIMS Version 6 data set Remsberg, Ellis Natarajan, Murali Harvey, V. Lynn 2018-09-09 application/pdf https://doi.org/10.5194/amt-11-3611-2018 https://amt.copernicus.org/articles/11/3611/2018/ eng eng doi:10.5194/amt-11-3611-2018 https://amt.copernicus.org/articles/11/3611/2018/ eISSN: 1867-8548 Text 2018 ftcopernicus https://doi.org/10.5194/amt-11-3611-2018 2020-07-20T16:23:13Z This study uses photochemical calculations along kinematic trajectories in conjunction with Limb Infrared Monitor of the Stratosphere (LIMS) observations to examine the changes in HNO 3 and NO 2 near 30 hPa in the region of the Aleutian High (AH) during the minor warming event of January 1979. An earlier analysis of Version 5 (V5) LIMS data indicated increases in HNO 3 without a corresponding decrease in NO 2 in that region and a quasi-wave 2 signature in the zonal distribution of HNO 3 , unlike the wave 1 signal in ozone and other tracers. Version 6 (V6) LIMS also shows an increase of HNO 3 in that region, but NO 2 is smaller than from V5. The focus here is to convey that V6 HNO 3 and NO 2 are of good quality, as shown by a re-examination of their mutual changes in the AH region. Photochemical model calculations initialized with LIMS V6 data show increases of about 2 ppbv in HNO 3 over 10 days along trajectories terminating in the AH region on 28 January. Those increases are mainly a result of the nighttime heterogeneous conversion of N 2 O 5 on background stratospheric sulfuric acid aerosols. Changes in the composition of the air parcels depend on the extent of exposure to sunlight and, hence, on the dynamically controlled history of the trajectories. Trajectories that begin in low latitudes and traverse to across the North Pole in a short time lead to the low HNO 3 in the region separating the anticyclone from the polar vortex, both of which contain higher HNO 3 . These findings help to explain the observed seasonal evolution and areal extent of both species. V6 HNO 3 and NO 2 are suitable, within their errors, for the validation of stratospheric chemistry–climate models. Text North Pole Copernicus Publications: E-Journals North Pole Atmospheric Measurement Techniques 11 6 3611 3626
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description This study uses photochemical calculations along kinematic trajectories in conjunction with Limb Infrared Monitor of the Stratosphere (LIMS) observations to examine the changes in HNO 3 and NO 2 near 30 hPa in the region of the Aleutian High (AH) during the minor warming event of January 1979. An earlier analysis of Version 5 (V5) LIMS data indicated increases in HNO 3 without a corresponding decrease in NO 2 in that region and a quasi-wave 2 signature in the zonal distribution of HNO 3 , unlike the wave 1 signal in ozone and other tracers. Version 6 (V6) LIMS also shows an increase of HNO 3 in that region, but NO 2 is smaller than from V5. The focus here is to convey that V6 HNO 3 and NO 2 are of good quality, as shown by a re-examination of their mutual changes in the AH region. Photochemical model calculations initialized with LIMS V6 data show increases of about 2 ppbv in HNO 3 over 10 days along trajectories terminating in the AH region on 28 January. Those increases are mainly a result of the nighttime heterogeneous conversion of N 2 O 5 on background stratospheric sulfuric acid aerosols. Changes in the composition of the air parcels depend on the extent of exposure to sunlight and, hence, on the dynamically controlled history of the trajectories. Trajectories that begin in low latitudes and traverse to across the North Pole in a short time lead to the low HNO 3 in the region separating the anticyclone from the polar vortex, both of which contain higher HNO 3 . These findings help to explain the observed seasonal evolution and areal extent of both species. V6 HNO 3 and NO 2 are suitable, within their errors, for the validation of stratospheric chemistry–climate models.
format Text
author Remsberg, Ellis
Natarajan, Murali
Harvey, V. Lynn
spellingShingle Remsberg, Ellis
Natarajan, Murali
Harvey, V. Lynn
On the consistency of HNO3 and NO2 in the Aleutian High region from the Nimbus 7 LIMS Version 6 data set
author_facet Remsberg, Ellis
Natarajan, Murali
Harvey, V. Lynn
author_sort Remsberg, Ellis
title On the consistency of HNO3 and NO2 in the Aleutian High region from the Nimbus 7 LIMS Version 6 data set
title_short On the consistency of HNO3 and NO2 in the Aleutian High region from the Nimbus 7 LIMS Version 6 data set
title_full On the consistency of HNO3 and NO2 in the Aleutian High region from the Nimbus 7 LIMS Version 6 data set
title_fullStr On the consistency of HNO3 and NO2 in the Aleutian High region from the Nimbus 7 LIMS Version 6 data set
title_full_unstemmed On the consistency of HNO3 and NO2 in the Aleutian High region from the Nimbus 7 LIMS Version 6 data set
title_sort on the consistency of hno3 and no2 in the aleutian high region from the nimbus 7 lims version 6 data set
publishDate 2018
url https://doi.org/10.5194/amt-11-3611-2018
https://amt.copernicus.org/articles/11/3611/2018/
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op_source eISSN: 1867-8548
op_relation doi:10.5194/amt-11-3611-2018
https://amt.copernicus.org/articles/11/3611/2018/
op_doi https://doi.org/10.5194/amt-11-3611-2018
container_title Atmospheric Measurement Techniques
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