Articles | Volume 20, issue 20
https://doi.org/10.5194/acp-20-12177-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
https://doi.org/10.5194/acp-20-12177-2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Ceilometers as planetary boundary layer height detectors and a corrective tool for COSMO and IFS models
Leenes Uzan
CORRESPONDING AUTHOR
Porter School of the Environment and Earth Sciences, Raymond and
Beverly Sackler Faculty of Exact Sciences, Dept. of Geophysics, Tel Aviv
University, Tel Aviv, 6997801, Israel
The Israeli Meteorological Service, Bet Dagan, Israel
Smadar Egert
Porter School of the Environment and Earth Sciences, Raymond and
Beverly Sackler Faculty of Exact Sciences, Dept. of Geophysics, Tel Aviv
University, Tel Aviv, 6997801, Israel
Pavel Khain
The Israeli Meteorological Service, Bet Dagan, Israel
Yoav Levi
The Israeli Meteorological Service, Bet Dagan, Israel
Elyakom Vadislavsky
The Israeli Meteorological Service, Bet Dagan, Israel
Pinhas Alpert
Porter School of the Environment and Earth Sciences, Raymond and
Beverly Sackler Faculty of Exact Sciences, Dept. of Geophysics, Tel Aviv
University, Tel Aviv, 6997801, Israel
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Latest update: 13 Nov 2024
Short summary
Detection of the planetary boundary layer (PBL) height is crucial to various fields, from air pollution assessment to weather prediction. We examined the diurnal summer PBL height by eight ceilometers in Israel, radiosonde profiles, the global IFS, and regional COSMO models. Our analysis utilized the bulk Richardson number method, the parcel method, and the wavelet covariance transform method. A novel correction tool to improve model results against in-situ ceilometer measurements is introduced.
Detection of the planetary boundary layer (PBL) height is crucial to various fields, from air...
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