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Automating Detection of the Planetary Boundary Layer in Aerosol Lidar Soundings. Virginia Sawyer Advisor: Dr. Judd Welton, NASA-GSFC. Planetary Boundary Layer. The transition between well-mixed surface air and the free atmosphere aloft.
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Automating Detection of the Planetary Boundary Layer in Aerosol Lidar Soundings Virginia Sawyer Advisor: Dr. Judd Welton, NASA-GSFC
Planetary Boundary Layer • The transition between well-mixed surface air and the free atmosphere aloft. • Usually maintained by a temperature inversion, which is buoyantly stable. • Important to air quality and climate modeling.
Entrainment Zone Frequently, the boundary layer is best expressed as a zone rather than a single height. This is especially true because of • Deep inversions with stably-stratified layers • Kelvin-Helmholz waves
LIDAR MPLNET is composed of micro pulse lidar sites, co-located with sunphotometers in the AERONET project, to provide continuous long-term data on atmospheric structure (primarily aerosol and clouds). Network includes sites from NASA and from partners around the world. The CALIPSO satellite contains a lidar and a wide field of view camera to study aerosol and clouds. CALIPSO is part of the A-train constellation in NASA’s Earth Observing System. 532 nm 523 or 527 nm
Wavelet Covariance Transform Haar Function a = width of entrainment zone b = PBL height Brooks, I.M., 2003. Finding Boundary Layer Top: Application of a Wavelet Covariance Transform to Lidar Backscatter Profiles. J. Atmos. Oceanic Technol. 20, 1092-1105.
MPLNET Goddard, 5/3/2001 Kelvin-Helmholz waves Elevated aerosol entrained by the PBL during the day Convective clouds Nighttime stable layers
Maximum of Wf(a,b) follows cloud deck
Program revised to follow aerosol layer below
CALIPSO 3:10-3:15 UTC 9/21/06 Particulate from South America?
CALIPSO 20:30-20:37 UTC 1/1/07 Himalayas
Conclusions • The wavelet covariance transform can be used to detect the planetary boundary layer in aerosol lidar soundings. • Modifications to the algorithm filter out high clouds and elevated aerosols, and speed up calculations. • Entrainment zone depth is more difficult to find in the relatively noisy CALIPSO data.
Thanks • Dr. Judd Welton, NASA • Larry Belcher, UMBC • Stephen Palm, SSAI • Research & Discover