Sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers

This work aims to assess differences in the aerosol optical depth (AOD) trend estimations when using high quality AOD measurements from two different instruments with different technical characteristics, operational (e.g. measurement frequency), calibration and processing protocols. The different ty...

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Main Authors: Karanikolas, Angelos, Kouremeti, Natalia, Gröbner, Julian, Egli, Luca, Kazadzis, Stelios
Format: Text
Language:English
Published: 2022
Subjects:
Online Access:https://doi.org/10.5194/amt-2022-181
https://amt.copernicus.org/preprints/amt-2022-181/
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spelling ftcopernicus:oai:publications.copernicus.org:amtd104554 2023-05-15T13:06:33+02:00 Sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers Karanikolas, Angelos Kouremeti, Natalia Gröbner, Julian Egli, Luca Kazadzis, Stelios 2022-07-04 application/pdf https://doi.org/10.5194/amt-2022-181 https://amt.copernicus.org/preprints/amt-2022-181/ eng eng doi:10.5194/amt-2022-181 https://amt.copernicus.org/preprints/amt-2022-181/ eISSN: 1867-8548 Text 2022 ftcopernicus https://doi.org/10.5194/amt-2022-181 2022-07-11T16:22:43Z This work aims to assess differences in the aerosol optical depth (AOD) trend estimations when using high quality AOD measurements from two different instruments with different technical characteristics, operational (e.g. measurement frequency), calibration and processing protocols. The different types of Sun photometers are the CIMEL that is part of AERONET (AErosol RObotic NETwork) and a precision Filter Radiometer (PFR), part of the Global Atmosphere Watch Precision Filter Radiometer network. The analysis operated for two wavelengths (500/501 nm and 870/862 nm for CIMEL/PFR) in Davos, Switzerland, for the period 2007–2019. For the synchronous AOD measurements, more than 95 % of the CIMEL-PFR AOD differences are within the WMO accepted limits, showing very good measurement agreement and homogeneity in calibration and post correction procedures. AOD trends per decade in AOD for Davos for the 13-year period of analysis were approximately -0.017 and -0.007 per decade for 501 nm and 862 nm (PFR), while the CIMEL-PFR trend differences have been found 0.0005 and 0.0003 respectively. The linear trend difference for 870/862 nm is larger than the linear fit standard error. When calculating monthly AODs using all PFR data (higher instrument frequency) and comparing them with the PFR measurements that are synchronous with CIMEL, the trend differences are smaller than the standard error. The trend differences are also larger than the trend uncertainty attributed to the instrument measurement uncertainty, with the exception of the comparison between the 2 PFR datasets (high and low frequency) at 862 nm. Finally, when calculating time-varying trends, they differ within their uncertainties. Text Aerosol Robotic Network Copernicus Publications: E-Journals
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description This work aims to assess differences in the aerosol optical depth (AOD) trend estimations when using high quality AOD measurements from two different instruments with different technical characteristics, operational (e.g. measurement frequency), calibration and processing protocols. The different types of Sun photometers are the CIMEL that is part of AERONET (AErosol RObotic NETwork) and a precision Filter Radiometer (PFR), part of the Global Atmosphere Watch Precision Filter Radiometer network. The analysis operated for two wavelengths (500/501 nm and 870/862 nm for CIMEL/PFR) in Davos, Switzerland, for the period 2007–2019. For the synchronous AOD measurements, more than 95 % of the CIMEL-PFR AOD differences are within the WMO accepted limits, showing very good measurement agreement and homogeneity in calibration and post correction procedures. AOD trends per decade in AOD for Davos for the 13-year period of analysis were approximately -0.017 and -0.007 per decade for 501 nm and 862 nm (PFR), while the CIMEL-PFR trend differences have been found 0.0005 and 0.0003 respectively. The linear trend difference for 870/862 nm is larger than the linear fit standard error. When calculating monthly AODs using all PFR data (higher instrument frequency) and comparing them with the PFR measurements that are synchronous with CIMEL, the trend differences are smaller than the standard error. The trend differences are also larger than the trend uncertainty attributed to the instrument measurement uncertainty, with the exception of the comparison between the 2 PFR datasets (high and low frequency) at 862 nm. Finally, when calculating time-varying trends, they differ within their uncertainties.
format Text
author Karanikolas, Angelos
Kouremeti, Natalia
Gröbner, Julian
Egli, Luca
Kazadzis, Stelios
spellingShingle Karanikolas, Angelos
Kouremeti, Natalia
Gröbner, Julian
Egli, Luca
Kazadzis, Stelios
Sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers
author_facet Karanikolas, Angelos
Kouremeti, Natalia
Gröbner, Julian
Egli, Luca
Kazadzis, Stelios
author_sort Karanikolas, Angelos
title Sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers
title_short Sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers
title_full Sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers
title_fullStr Sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers
title_full_unstemmed Sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers
title_sort sensitivity of aerosol optical depth trends using long term measurements of different sun-photometers
publishDate 2022
url https://doi.org/10.5194/amt-2022-181
https://amt.copernicus.org/preprints/amt-2022-181/
genre Aerosol Robotic Network
genre_facet Aerosol Robotic Network
op_source eISSN: 1867-8548
op_relation doi:10.5194/amt-2022-181
https://amt.copernicus.org/preprints/amt-2022-181/
op_doi https://doi.org/10.5194/amt-2022-181
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