The Mid-latitude Continental Convective Clouds Experiment ...
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The Mid-latitude Continental Convective Clouds Experiment (MC3E) M. Jensen 1 , W. Petersen 2 , N. Bharadwaj 3 , A. Del Genio 4 , S. Giangrande 1 , D. Hartsock 5 , A. Heymsfield 6 , G. Heymsfield 7 , A. Hou 7 , P. Kollias 8 , P. Lamb 5 , B. Orr 9 , S. Rutledge 10 , M. Schwaller 7 , D. Sisterson 9 , E. Zipser 11 1 BNL, 2 NASA MSFC, 3 PNNL, 4 NASA GISS, 5 U. Oklahoma, 6 NCAR, 7 NASA GSFC, 8 McGill U., 9 ANL, 10 CSU, 11 U. of Utah MC3E April 22 – June 6 ARM Southern Great Plains Central Facility Represents a collaborative effort between the DOE ASR Program and the NASA Global Precipitation Measurement (GPM) mission Overarching Science : A complete characterization of convective cloud systems in order to: 1) Advance the understanding of the different components of convective parameterization • Focus: Convective initiation and up/downdraft coupling to precipitation and cloud microphysics. 2) Improve the fidelity of satellite estimates of precipitation over land. • Focus: Observation and quantification of dominant column microphysical processes impacting satellite-based passive/active microwave retrievals AMPR (Passive) H+V polarizations Characteristics Frequencies 10.7, 19.35, 37.1, 85.5 GHz Resolution @ 20 km range 0.6 km (85.5 GHz), 1.5 km (37.1 GHz), 2.8 km (10.7-19.35 GHz) CoSMIR (Passive) H+V polarizations Frequencies 37, 89, 165.5, 183.3+/-1, 183.3+/-3, 183.3+/-8 GHz Resolution @ 20 km range 1.4 km footprint at nadir HIWRAP Ka-Ku band (Active) Frequency (inner/outer beam) 13.91/13.35 GHz, 35.56/33.72 GHz Transmit peak power 30 W (Ku), 10 W (Ka) 3 dB beamwidth 2.9º Ku, 1.2º Ka MDS (dBZ e , 60 m res., 3.3 ms chirp pulse, 10 km range) 0.0, -5.0 dBZ e CRS W-band (Active) Frequency 94.15 GHz (dual- polarized) Transmit peak power 1700 W 3 dB beamwidth 0.6º x 0.8º MDS (dBZ e , 0.5 ms pulse; 1 km range) -35 dBZ e NASA ER-2 Radiometer and Radars MC3E Airborne Instrumentation Instruments Measurement FSSP/King Cloud liquid water PMS or DMT (TBD: 2D-C/P, CIP/PIP etc.) Cloud and precipitation particle spectra SPEC Inc. HVPS Large hydrometeor spectra SPEC Inc. 2D-S Cloud particle spectra CDP and/or SID Cloud particle spectra CVI Total water content Rosemount icing probe Supercooled liquid water CN counter (10 nm cut), UHSAS (100 channels, 60 nm – 1 micron) CN/CCN UND Citation Multi-frequency, Multi-scale Radar-based • X-band radar network (X-SAPR) • NASA S-Band Transportable Dual-Polarimetric Radar (NPOL) • C-band (Dual Polarization) Scanning ARM Precipitation Radar (C- SAPR) • NASA Ka/Ku band Deployable Dual-Polarimetric Doppler Scanning Radar (D3R) • ARM Dual-Wavelength (Ka/W) Scanning Cloud Radar (Ka-SACR/W- SACR) •NOAA-ESRL S-Band and 449 MHz Profiler Pair • ARM 915 MHz Wind Profilers • National Weather Service WSR-88Ds • NOAA Profiler Network 404 MHz Wind Profilers Radiosonde Array • Six launch sites • Pratt, KS • Chanutte, KS • Vici, OK • Morris, OK • Purcell, OK •Lamont, OK • Launch Frequency 4-8x per day NASA Disdrometer Facility • 16 Parsivel disdrometers • 5 3 rd -generation 2D Video Disdrometers • 20 Rain gauges Campaign Measurement Objectives DOE ASR 1) Determine Pre-convective environment, large-scale fording and feedbacks 2) Observations of convective initiation, 3) Quantify updraft / downdraft dynamics, 4) Diagnose Condensate transport / detrainment / entrainment 5) Characterize precipitation and cloud microphysics, 6) Assess influences on radiation NASA GPM 1) Coordinated airborne “satellite simulator” and in-situ platform a. High-altitude Ka/Ku-band radar + multi-frequency radiometer overflying in-situ ice microphysics aircraft 2) Unified 3-D Mapping of hydrometeor distribution/type a. Sub pixel-scale DSD and rain rate variability (0.5 – 5 km) 3) Data to support satellite simulator model testing (CRM/LSM/RT) a. Collection of high quality sounding-based forcing data sets b. Microphysical and kinematic validation datasets. c. Land surface states affecting variability in emission. Contacts Michael Jensen, [email protected] Walt Petersen, [email protected] MC3E “dream” scenario
Transcript of The Mid-latitude Continental Convective Clouds Experiment ...
The Mid-latitude Continental Convective Clouds Experiment (MC3E)M. Jensen1, W. Petersen2, N. Bharadwaj3, A. Del Genio4, S. Giangrande1, D. Hartsock5, A. Heymsfield6, G. Heymsfield7, A. Hou7, P. Kollias8, P. Lamb5, B. Orr9,
S. Rutledge10, M. Schwaller7, D. Sisterson9, E. Zipser11
1BNL, 2NASA MSFC, 3PNNL, 4NASA GISS, 5U. Oklahoma, 6NCAR, 7NASA GSFC, 8 McGill U., 9 ANL,10 CSU, 11U. of Utah
MC3E April 22 – June 6 ARM Southern Great Plains Central Facility
Represents a collaborative effort between the DOE ASR Program and the NASA Global Precipitation Measurement (GPM) mission
Overarching Science:A complete characterization of convective cloud systems in order to:
1) Advance the understanding of the different components of convective parameterization• Focus: Convective initiation and up/downdraft coupling to
precipitation and cloud microphysics.
2) Improve the fidelity of satellite estimates of precipitation over land.
• Focus: Observation and quantification of dominant column microphysical processes impacting satellite-based passive/active microwave retrievals
AMPR (Passive) H+V
polarizations
Characteristics
Frequencies 10.7, 19.35, 37.1, 85.5
GHz
Resolution @ 20 km
range
0.6 km (85.5 GHz), 1.5
km (37.1 GHz), 2.8 km
(10.7-19.35 GHz)
CoSMIR (Passive) H+V
polarizations
Frequencies 37, 89, 165.5, 183.3+/-1,
183.3+/-3, 183.3+/-8 GHz
Resolution @ 20 km
range
1.4 km footprint at nadir
HIWRAP Ka-Ku band
(Active)
Frequency (inner/outer
beam)
13.91/13.35 GHz,
35.56/33.72 GHz
Transmit peak power 30 W (Ku), 10 W (Ka)
3 dB beamwidth 2.9º Ku, 1.2º Ka
MDS (dBZe, 60 m res.,
3.3 ms chirp pulse, 10
km range)
0.0, -5.0 dBZe
CRS W-band (Active)
Frequency 94.15 GHz (dual-
polarized)
Transmit peak power 1700 W
3 dB beamwidth 0.6º x 0.8º
MDS (dBZe, 0.5 ms
pulse; 1 km range)
-35 dBZe
NASA ER-2 Radiometer and Radars
MC3E Airborne Instrumentation
Instruments Measurement
FSSP/King Cloud liquid water
PMS or DMT (TBD:
2D-C/P, CIP/PIP
etc.)
Cloud and
precipitation particle
spectra
SPEC Inc. HVPS Large hydrometeor
spectra
SPEC Inc. 2D-S Cloud particle spectra
CDP and/or SID Cloud particle spectra
CVI Total water content
Rosemount icing
probe
Supercooled liquid
water
CN counter (10 nm
cut), UHSAS (100
channels, 60 nm – 1
micron)
CN/CCN
UND Citation
Multi-frequency, Multi-scale Radar-based• X-band radar network (X-SAPR)
• NASA S-Band Transportable Dual-Polarimetric Radar (NPOL)• C-band (Dual Polarization) Scanning ARM Precipitation Radar (C-SAPR)• NASA Ka/Ku band Deployable Dual-Polarimetric Doppler Scanning Radar (D3R)• ARM Dual-Wavelength (Ka/W) Scanning Cloud Radar (Ka-SACR/W-SACR)•NOAA-ESRL S-Band and 449 MHz Profiler Pair• ARM 915 MHz Wind Profilers• National Weather Service WSR-88Ds• NOAA Profiler Network 404 MHz Wind Profilers
Radiosonde Array• Six launch sites
• Pratt, KS• Chanutte, KS• Vici, OK• Morris, OK• Purcell, OK•Lamont, OK
• Launch Frequency 4-8x per day
NASA Disdrometer Facility• 16 Parsivel disdrometers• 5 3rd-generation 2D Video Disdrometers• 20 Rain gauges
Campaign Measurement Objectives DOE ASR1) Determine Pre-convective environment, large-scale fording and
feedbacks2) Observations of convective initiation, 3) Quantify updraft / downdraft dynamics, 4) Diagnose Condensate transport / detrainment / entrainment 5) Characterize precipitation and cloud microphysics, 6) Assess influences on radiation
NASA GPM1) Coordinated airborne “satellite simulator” and in-situ platform
a. High-altitude Ka/Ku-band radar + multi-frequency radiometer overflying in-situ ice microphysics aircraft
2) Unified 3-D Mapping of hydrometeor distribution/typea. Sub pixel-scale DSD and rain rate variability (0.5 – 5 km)
3) Data to support satellite simulator model testing (CRM/LSM/RT) a. Collection of high quality sounding-based forcing data sets b. Microphysical and kinematic validation datasets. c. Land surface states affecting variability in emission.
ContactsMichael Jensen, [email protected]
Walt Petersen, [email protected]
MC3E “dream” scenario
