Abstract:Abstract. Aerosol layer height is an essential parameter to understand the impact of aerosols on the climate system. As part of the European Space Agency Aerosol_cci project, aerosol layer height as derived from passive thermal and solar satellite sensors measurements, have been compared with aerosol layer heights estimated from CALIOP measurements. The Aerosol_cci project targeted dust type aerosol for this study. This ensures relatively unambiguous aerosol identification by the CALIOP processing chain. Dust … Show more
“…In the same study, spatial distributions of AOD have also been compared to MODIS/TERRA and Spinning Enhanced Visible and Infrared Imager (SEVIRI), showing a strong consistency. Still at daily scale, IASI altitudes have been compared with CALIOP mean altitudes (Kylling et al, 2018). Comparisons with CALIOP are not easy to interpret, given the different characteristics of the two instruments: much higher vertical resolution of CALIOP (IASI provides information on the atmospheric vertical structure with a resolution of ~1 km in the lower troposphere to 2 km in the free troposphere, Chalon et al, 2001; see also the iasi.cnes.fr/en and https://www.eumetsat.int websites), observation times differing by about 4 hr, difference in the altitude definition, difference in the spatial resolution, low CALIOP repeat cycle of 16 days, lower CALIOP daytime signal‐to‐noise ratio.…”
Section: Determination Of Dust Aod and Altitude From Iasi Observationsmentioning
Observing the planet at global scale, twice a day, and measuring the whole infrared atmospheric spectrum (8,461 channels at 0.50 cm−1 resolution), Infrared Atmospheric Sounder Interferometer (IASI)/METOP can concurrently detect clouds, determine the 3‐D atmospheric structure (temperature, water vapor, ozone, etc.), surface properties (emissivity and temperature), as well as dust aerosol AOD and altitude. Observing morning (0930 hr) and nighttime (2130 hr), IASI is in relatively good phase with the most frequent times of occurrence of the main Saharan dust uplift mechanisms reported in the literature. Here we classify IASI dust observations according to both the dust loading (AOD) and the dust layer height, providing a more comprehensive picture of dust characteristics. This classification is analyzed at daily scale and its capability to detect dust uplift events is evaluated through comparisons with results from the particularly well documented June 2011 Fennec campaign. Then, a Dust Emission Index (DEI), specific to IASI, is constructed by selecting AOD‐altitude bins with largest AODs and smallest altitudes likely indicative of freshly emitted dust. Applying this to the 12‐year 2007–2018 period, we determine climatological DEI maps and comparisons are made with other equivalent existing results derived from ground‐based or other satellite observations. Results of these comparisons demonstrate the capability of IASI to document the dust distribution over the whole Earth desert areas over a long period of time. The present approach is also suitable to the processing of the at least hourly observations of the coming Infrared Sounder instrument (IRS), planned on board Meteosat Third Generation (2021).
“…In the same study, spatial distributions of AOD have also been compared to MODIS/TERRA and Spinning Enhanced Visible and Infrared Imager (SEVIRI), showing a strong consistency. Still at daily scale, IASI altitudes have been compared with CALIOP mean altitudes (Kylling et al, 2018). Comparisons with CALIOP are not easy to interpret, given the different characteristics of the two instruments: much higher vertical resolution of CALIOP (IASI provides information on the atmospheric vertical structure with a resolution of ~1 km in the lower troposphere to 2 km in the free troposphere, Chalon et al, 2001; see also the iasi.cnes.fr/en and https://www.eumetsat.int websites), observation times differing by about 4 hr, difference in the altitude definition, difference in the spatial resolution, low CALIOP repeat cycle of 16 days, lower CALIOP daytime signal‐to‐noise ratio.…”
Section: Determination Of Dust Aod and Altitude From Iasi Observationsmentioning
Observing the planet at global scale, twice a day, and measuring the whole infrared atmospheric spectrum (8,461 channels at 0.50 cm−1 resolution), Infrared Atmospheric Sounder Interferometer (IASI)/METOP can concurrently detect clouds, determine the 3‐D atmospheric structure (temperature, water vapor, ozone, etc.), surface properties (emissivity and temperature), as well as dust aerosol AOD and altitude. Observing morning (0930 hr) and nighttime (2130 hr), IASI is in relatively good phase with the most frequent times of occurrence of the main Saharan dust uplift mechanisms reported in the literature. Here we classify IASI dust observations according to both the dust loading (AOD) and the dust layer height, providing a more comprehensive picture of dust characteristics. This classification is analyzed at daily scale and its capability to detect dust uplift events is evaluated through comparisons with results from the particularly well documented June 2011 Fennec campaign. Then, a Dust Emission Index (DEI), specific to IASI, is constructed by selecting AOD‐altitude bins with largest AODs and smallest altitudes likely indicative of freshly emitted dust. Applying this to the 12‐year 2007–2018 period, we determine climatological DEI maps and comparisons are made with other equivalent existing results derived from ground‐based or other satellite observations. Results of these comparisons demonstrate the capability of IASI to document the dust distribution over the whole Earth desert areas over a long period of time. The present approach is also suitable to the processing of the at least hourly observations of the coming Infrared Sounder instrument (IRS), planned on board Meteosat Third Generation (2021).
“…Although coverage by these measurements is currently limited, their precision has demonstrated value in constraining and/or validating models aimed at simulating downwind wildfire smoke and volcanic ash dispersion (e.g., Zhu et al, 2018a;Vernon et al, 2018). A number of satellite-based, passive-imager spectral techniques, at wavelengths ranging from the ultraviolet (UV) to the infrared, offer greater aerosol layer-height coverage, at the cost of additional assumptions that increase uncertainty (e.g., Jeong & Hsu, 2008, Griffin et al, 2020Go et al, 2020;Kylling et al, 2018;Lu et al, 2021;Lyapustin et al, 2020). Passive-imager techniques, especially in UV channels, have also been effective in constraining aerosol occurrence, and even amount, over cloudy scenes (e.g., Torres et al, 2012;Meyer et al, 2015;Sayer et al, 2019).…”
Aerosol forcing uncertainty represents the largest climate forcing uncertainty overall. Its magnitude has remained virtually undiminished over the past 20 years despite considerable advances in understanding most of the key contributing elements. Recent work has produced modest increases only in the confidence of the uncertainty estimate itself. This review summarizes the contributions toward reducing the uncertainty in the aerosol forcing of climate made by satellite observations, measurements taken within the atmosphere, as well as modeling and data assimilation. We adopt a more measurement‐oriented perspective than most reviews of the subject in assessing the strengths and limitations of each; gaps and possible ways to fill them are considered. Currently planned programs supporting advanced, global‐scale satellite and surface‐based aerosol, cloud, and precursor gas observations, climate modeling, and intensive field campaigns aimed at characterizing the underlying physical and chemical processes involved, are all essential. But in addition, new efforts are needed: (a) to obtain systematic aircraft in situ measurements capturing the multi‐variate probability distribution functions of particle optical, microphysical, and chemical properties (and associated uncertainty estimates), as well as co‐variability with meteorology, for the major aerosol airmass types; (b) to conceive, develop, and implement a suborbital (aircraft plus surface‐based) program aimed at systematically quantifying the cloud‐scale microphysics, cloud optical properties, and cloud‐related vertical velocities associated with aerosol‐cloud interactions; and (c) to focus much more research on integrating the unique contributions of satellite observations, suborbital measurements, and modeling, to reduce the persistent uncertainty in aerosol climate forcing.
“…Beyond its climatological value, our CALIPSO dust product has been utilized to study the physics of the dust cycle in the atmosphere (Georgoulias et al 2016;Solomos et al 2017;Kosmopoulos et al 2017;Amiri-Farahani et al 2017;Kylling et al 2017).…”
Section: Chapter Appendix: Use Of Calipso Dust Product For Comparison Studiesmentioning
Ο πρωταρχικός στόχος αυτής της εργασίας είναι να καλύψει υπάρχοντα κενά στην αντίληψή μας σχετικά με το ρόλο της ερημικής σκόνης στις κλιματικές παραμέτρους της Μεσογείου χρησιμοποιώντας προηγμένες μεθόδους τηλεπισκόπησης. Αρχικά, η ερημική σκόνη διαχωρίζεται από τα συνολικά αερολύματα που παρέχονται από σύγχρονους δορυφορικούς αισθητήρες τηλεπισκόπησης. Το προϊόν σκόνης που παράγεται χρησιμοποιείται στην ανάπτυξη της τρισδιάστατης κατανομής του φόρτου της σκόνης πάνω από τη Μεσόγειο και τη Βόρεια Αφρική, η οποία είναι πολύ σημαντική για την επίδραση της σκόνης στην ηλιακή ακτινοβολία. Τέλος, αναπτύσσουμε κλιματολογίες των συγκεντρώσεων της σκόνης που ενεργούν ως πυρήνες παγoποίησης, για τη μελέτη της επίδρασης της σκόνης στο σχηματισμό νεφών.Η μεθοδολογία μας περιλαμβάνει τη συνέργεια παθητικών και ενεργών μετρήσεων τηλεπισκόπησης, με έμφαση στις κατακόρυφες μετρήσεις των αερολυμάτων που παρέχονται από το δορυφορικό lidar του CALIPSO (Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations). Αρχικά, αναπτύσσουμε ένα νέο προϊόν σκόνης χρησιμοποιώντας τις μετρήσεις του CALIPSO, βασιζόμενοι σε μεθοδολογίες που έχουν αναπτυχθεί στο πλαίσιο του Ευρωπαικού επίγειου δικτύου lidar EARLINET (AErosol RObotic NETwork). Ο διαχωρισμός της σκό-νης από τους άλλους τύπους αερολυμάτων γίνεται χρησιμοποιώντας τα προφίλ του συντελεστή οπισθοσκέδασης και του λόγου αποπόλωσης του CALIPSO, καθώς και τις μετρήσεις και τις μεθόδους του EARLINET. Το προϊόν αξιολογείται με μετρήσεις από το δίκτυο AERONET (AEr-osol RObotic NETwork) και συγκρίνεται με δορυφορικές παρατηρήσεις από το MODIS (Moderate Resolution Imaging Spectroradiometer) και με κατακόρυφα προφίλ από το μοντέλο BSC-DREAM8b (Barcelona Supercomputer Center - Dust Regional Atmospheric Model). Το νέο προϊόν σκόνης χρησιμοποιείται για την παραγωγή μιας τρισδιάστατης κλιματολογίας της εξέλιξης της Σαχαριανής σκόνης πάνω από την Βόρεια Αφρική και την Ευρώπη, χρησιμοποιώντας τις δορυφορικές παρατηρήσεις του CALIPSO από το 2007 έως το 2015. Τα αποτελέσματα αναδεικνύουν την τρισδιάστατη εξέλιξη της σκόνης και τις εποχιακές διαδρομές της μεταφοράς της από τη Σαχάρα προς τη Μεσόγειο και την ηπειρωτική Ευρώπη. Το νέο προϊόν σκόνης είναι ελεύθερα διαθέσημο (κατόπιν αιτήσεως αλλά και από διάφορες ιστοσελίδες) και έχει ήδη χρησιμοποιηθεί από την παγκόσμια μετεωρολογική οργάνωση, την ευρωπαϊκή υπηρεσία διαστήματος και από συνεργάτες ερευνητές για την αξιολόγηση 3 μοντέλων μεταφοράς σκόνης, νέων προϊόντων από δορυφόρους πολικής και γεωστατικής τροχιάς και για την μελέτη της επίδρασης της σκόνης στο ισοζύγιο της ακτινοβολίας. Εδώ παρουσιάζονται τρία παραδείγματα τέτοιων εφαρμογών, με πρώτο (α) τη βελτιστοποίηση των παραμέτρων ενός μοντέλου μεταφοράς σκόνης προκειμένου να περιγραφεί η καταιγίδα σκόνης στη Μέση Ανατο-λή και την Ανατολική Μεσόγειο συνέβει το 2015, β) την κατηγοριοποίηση αερολυμάτων από το διάστημα με σκοπό τον διαχωρισμό των αερολυμάτων ανθρωπογενούς και φυσικής προέλευσης και (γ) την αξιολόγηση διαφορετικών παραμετροποιήσεων σκόνης σε περιφερειακά κλιματικά μοντέλα. Τέλος, ανακτώνται οι κατακόρυφες κατανομές συγκέντρωσης πυρήνων παγοποίησης στην περιοχή της μελέτης. Αυτό το αποτέλεσμα παρέχει μια μοναδική ευκαιρία για μελλοντική έρευνα πάνω στον ετερογενή σχηματισμού του πάγου, χρησιμοποιώντας παρατηρήσεις νεφών.
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