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APOLLO_NG - a probabilistic interpretation of the APOLLO legacy for AVHRR heritage channels

Klüser, Lars und Killius, Niels und Gesell, Gerhard (2015) APOLLO_NG - a probabilistic interpretation of the APOLLO legacy for AVHRR heritage channels. Atmospheric Measurement Techniques, 8, Seiten 4155-4170. Copernicus Publications. doi: 10.5194/amt-8-4155-2015. ISSN 1867-1381.

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Offizielle URL: http://www.atmos-meas-tech.net/8/4155/2015/

Kurzfassung

The cloud processing scheme APOLLO (AVHRR Processing scheme Over cLouds, Land and Ocean) has been in use for cloud detection and cloud property retrieval since the late 1980s. The physics of the APOLLO scheme still build the backbone of a range of cloud detection algorithms for AVHRR (Advanced Very High Resolution Radiometer) heritage instruments. The APOLLO_NG (APOLLO_NextGeneration) cloud processing scheme is a probabilistic interpretation of the original APOLLO method. It builds upon the physical principles that have served well in the original APOLLO scheme. Nevertheless, a couple of additional variables have been introduced in APOLLO_NG. Cloud detection is no longer performed as a binary yes/no decision based on these physical principles. It is rather expressed as cloud probability for each satellite pixel. Consequently, the outcome of the algorithm can be tuned from being sure to reliably identify clear pixels to conditions of reliably identifying definitely cloudy pixels, depending on the purpose. The probabilistic approach allows retrieving not only the cloud properties (optical depth, effective radius, cloud top temperature and cloud water path) but also their uncertainties. APOLLO_NG is designed as a standalone cloud retrieval method robust enough for operational near-realtime use and for application to large amounts of historical satellite data. The radiative transfer solution is approximated by the same two-stream approach which also had been used for the original APOLLO. This allows the algorithm to be applied to a wide range of sensors without the necessity of sensorspecific tuning. Moreover it allows for online calculation of the radiative transfer (i.e., within the retrieval algorithm) giving rise to a detailed probabilistic treatment of cloud variables. This study presents the algorithm for cloud detection and cloud property retrieval together with the physical principles from the APOLLO legacy it is based on. Furthermore a couple of example results from NOAA-18 are presented.

elib-URL des Eintrags:https://elib.dlr.de/99263/
Dokumentart:Zeitschriftenbeitrag
Titel:APOLLO_NG - a probabilistic interpretation of the APOLLO legacy for AVHRR heritage channels
Autoren:
AutorenInstitution oder E-Mail-AdresseAutoren-ORCID-iDORCID Put Code
Klüser, LarsDFDNICHT SPEZIFIZIERTNICHT SPEZIFIZIERT
Killius, NielsDFDNICHT SPEZIFIZIERTNICHT SPEZIFIZIERT
Gesell, GerhardDFDNICHT SPEZIFIZIERTNICHT SPEZIFIZIERT
Datum:12 Oktober 2015
Erschienen in:Atmospheric Measurement Techniques
Referierte Publikation:Ja
Open Access:Ja
Gold Open Access:Ja
In SCOPUS:Ja
In ISI Web of Science:Ja
Band:8
DOI:10.5194/amt-8-4155-2015
Seitenbereich:Seiten 4155-4170
Verlag:Copernicus Publications
ISSN:1867-1381
Status:veröffentlicht
Stichwörter:AVHRR Clouds Remote Sensing Cloud detection APOLLO
HGF - Forschungsbereich:Luftfahrt, Raumfahrt und Verkehr
HGF - Programm:Raumfahrt
HGF - Programmthema:Erdbeobachtung
DLR - Schwerpunkt:Raumfahrt
DLR - Forschungsgebiet:R EO - Erdbeobachtung
DLR - Teilgebiet (Projekt, Vorhaben):R - Fernerkundung u. Geoforschung
Standort: Oberpfaffenhofen
Institute & Einrichtungen:Deutsches Fernerkundungsdatenzentrum > Atmosphäre
Hinterlegt von: Klüser, Dr. Lars
Hinterlegt am:10 Nov 2015 11:27
Letzte Änderung:27 Nov 2023 14:23

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