marine boundary layer cloud-top-height from …...marine boundary layer cloud-top-height from modis,...
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Marine Boundary Layer Cloud-top-height from MODIS, CALIPSO and COSMIC Over
Subtropical Eastern Oceans
Feiqin Xie
Department of Physical & Environmental Sciences Texas A&M University – Corpus Christi
Coauthors: L. Adhikari (TAMUCC), D. L. Wu (GSFC), R. Wood (UW)
Acknowledgement: NASA-NNX14AK17G (Dr. Ramesh Kakar)
MODIS Science Team Meeting, Silver Spring, MD
May 20, 2015 1
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Liquid water cloud fraction – Aqua
Six selected regions with prevailing boundary layer clouds.
[King et al., 2013]
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Trade cumuli Stratocumulus
GOES
Transition
Bo4om photographs courtesy of Dr. Bjorn Stevens
Marine Atmospheric Boundary Layer Clouds
Cloud photos courtesy of Dr. B. Stevens 3
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Lock et al., 2000, MWR
Different Cloudy Boundary Layer Structure
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MBL Height Measurement
• Vertical profiling – Balloon sounding – profiling (T/q) – GPS radio occultation (refractivity, bending angle)
• MBL-top tracer tracking – CALIPSO lidar, clouds and aerosol backscattering – MODIS, cloud-top-temperature, cloud fraction – Limitation: only works when tracers are available
• MODIS lapse-rate method (Zuidema et al., 2009)
– ΓT =6.9 (K/km) is the lapse rate, – δT=2.35 (K) is the temperature bias adjustment
CTH =(SST −CTT )−δT
ΓT
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Stratocumulus-topped MBL
VAMOS Ocean-Cloud-Atmosphere-Land Study (2008-Oct-Nov)
VOCALS
Temp
q
Temp
q
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The inversion-base height is consistent with Cloud-top-height Lower boundary layer height à lower clouds
Courtesy of Prof. R. Wood Univ. of Washington
VOCALS MBL Structure
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Neutral atmosphere
(Below ~70 km)
Ionosphere
Figure Courtesy of UCAR COSMIC Group
GPS Radio Occultation
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Near-coincident COSMIC vs. CALIPSO (<18min apart)
GOES
COSMIC vs. CALIPSO
20S
24S
74W 76W
CALIPSO
22S
18S
72W 78W
COSMIC/RO
26S
Near-coincident COSMIC vs. CALIPSO (<18min apart)
Bending Angle
Refractivity Gradient
ECMWF
ECMWF
GOES
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CALIPSO
CALIPSO
COSMIC
Tdry Bend
CALIPSO
2008-‐07-‐27
Height (km)
Tdry = a1*P / N
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MODIS Cloud Measurement
Cloud-top-temperature (K) Cloud Fraction (%)
COSMIC/RO
CALIPSO
CTH =(SST −CTT )−δT
ΓT 11
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MODIS Cloud-top-height
CTTMODIS
CTHMODIS
CTHCALIPSO
CALIPSO
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MODIS-CTH - Lapse rate
CTHMODIS l Lapse Rate (LR)
l Cloud Fraction (CF) CTHCALIPSO
GPS (20.34°S, 74.28°W)
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MODIS Cloud-top-height
COSMIC/RO
CALIPSO
MODIS Lapse Rate CTH & Cloud Fraction CTH Difference: CTHLapseRate – CTHMODIS-V6
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!
JJA
SON
CALIPSO-CTH COSMIC-PBLH
Cloud-Top-Height vs. MBL Height
PBLH-CTH 2007-‐2010
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Conclusions and Future Works
" MODIS cloud-‐top-‐temperature (CTT) along with SST can be used to derive the cloud-‐top-‐height (CTH) based on the lapse rate method.
" CALIPSO Cloud-‐top-‐height climatology compares well with COSMIC GPS RO with best agreement over stratocumulus region (<200 m) near the coast of subtropical eastern Pacific ocean.
" Significant discrepancy is found over tropical and trade wind region, where broken clouds and weaker boundary layer inversion and moisture gradient complicate the detecXon of CTH from CALIPSO lidar and GPS RO measurements, respecXvely.
" The lapse rate method is sensiXve to the lapse rate and the cloud fracXon. More robust retrieval algorithm need to be developed to offer best quality CTH retrieval.
" CALIPSO and GPS RO offer independent CTH measurements and will be used to verify and improve the MODIS CTH retrieval, which will be used to derive cloud top entrainment rate given the cloud top wind and large-‐scale subsidence rate esXmaXon.
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Acknowledgement • Supported by NASA-NNX14AK17G, special thanks to Dr. Ramesh
Kakar. • JPL GPS operational team: C. O. Ao, A. J. Mannucci, B. Iijima, M.
Pestanal, T. Meehan and L. E. Young for COSMIC RO soundings. • UCAR COSMIC Group for UCAR COSMIC retrievals • ECMWF/ERA-interim data • CALIPSO data These data were obtained from the NASA Langley
Research Center Atmospheric Science Data Center.
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