UTLS - Science - DC3 Field Campaign
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Deep Convective Clouds & Chemistry
Experiment (DC3) |
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Principal Investigators
Contact PI:
Mary Barth
NCAR- ACD
303-497-8186
William Brune
PSU
814-865-3286
Chris Cantrell
NCAR- ACD
303-497-1479
Steven Rutledge
CSU
970-491-8283
Steering Committee
(includes those above)
Jim Crawford
NASA-Langley
757-864-7231
Owen Cooper
NOAA- CSD &
CU-CIRES
303-497-3599
Alan Fried
NCAR-EOL
303-497-1475
Andrew Heymsfield
NCAR-MMM
303-497-8943
Paul Krehbiel
NMT
505-835-5215
Donald Lenschow
NCAR-MMM
303-497-8903
Laura Pan
NCAR-ACD &
NCAR-TIIMES
303-497-1467
Kenneth Pickering
NASA-Goddard
301-405-7639
Jeffrey Stith
NCAR-EOL
303-497-1032
Andy Weinheimer
NCAR-ACD
303-497-1444 |
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The DC3 Field Experiment will characterize the effect of midlatitude, continental
convection on the transport and transformation of ozone and its precursors. Along with
measurements of hydrogen oxide radicals, their precursors, and nitrogen oxides in both
the inflow and outflow regions of deep convection, measurements of cloud microphysical
properties, storm kinematics, and lightning discharges will be conducted. These
measurements are planned for the central United States during summer 2010 where remote
continental regions can be contrasted to anthropogenically-influenced regions.
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Motivation |
Ozone in the UTLS region is important for climate change and for affecting the UV radiation reaching the Earth's surface.
Ozone is produced from NOx and HOx radicals. Thus, quantifying the sources of NOx and HOx in the upper troposphere is key to understanding the climate implications of upper tropospheric O3.
Deep convection alters the composition of the UTLS region.
Important precursors of O3 are NOx, HOx, and the HOx precursors.
DC3 will give us:
- Comprehensive chemistry on board NSF/NCAR HIAPER and NASA DC-8 aircraft
- Comprehensive storm information from ground-based Doppler and polarimetric radars
- Outstanding information on lightning location from lightning mapping arrays
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Science Goals |
Quantify the impact of continental, midlatitude convective storm dynamics, multiphase chemistry, lightning, and physics on the transport of chemical constituents to the upper troposphere
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Can we locate the source of NO within the storm in relation to the kinematics, and the location of the lightning and microphysical structure?
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Can we determine the production of NOx from intracloud lightning in relation to that from cloud-to-ground lightning?
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Determine the mass fluxes of air and trace gases into and out of the storm, including entrainment from the boundary layer, mid-troposphere, and stratosphere
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What fraction of the boundary layer air reaches the upper troposphere?
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What’s the degree of entrainment?
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What part of the boundary layer is ingested into the storm?
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Determine the effects of convectively-perturbed air masses on ozone and its related chemistry in the midlatitude upper troposphere and lower stratosphere near the convective cores (in the anvil region) and further downwind, 12-48 hours after the near convection region is sampled
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In the anvil, does the scattering of actinic fluxes significantly affect concentrations?
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What role does adsorption of gases onto ice play in affecting the chemistry?
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What chemical aging occurs in the convective outflow? Is O3 produced (and how much)?
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Contrast the influence of different surface emission rates on the composition of convective outflow
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Is more O3 produced in convective outflow when the convection occurs over relatively clean regions?
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What is the importance of biogenic hydrocarbons (e.g. isoprene) on the chemical aging in convective outflow regions?
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Ancillary Goals |
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To improve our understanding of cloud electrification and lightning discharge processes (in relation to NO production; contrasting differences among different convective regimes)
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To investigate the role of deep convection in contributing to the UT water vapor and in the transport of water vapor into the lowermost stratosphere
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To connect aerosol and cloud droplet and ice particle number concentrations with convection characteristics and trace gas convective processing
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To determine partitioning of reactive halogen and reservoir species in the UTLS
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Experimental Design |

High Altitude Aircraft
(e.g. NSF/NCAR G-V)
outfitted with gas-phase and aerosol characterization instrumentation to sample convective outflow |
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Low Altitude Aircraft
(e.g. NASA DC-8) configured with in situ and remote gas, aerosol, liquid and ice characterization instruments to sample inflow region, mid-troposphere, and locate downwind plumes |
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Ground based facilities
To measure winds, hydrometeors, lightning characteristics, thermodynamics, and species profiles
Utilize (existing) ground based networks to sample in diverse precipitation, lightning and background chemistry regimes: |

Northeast Colorado
- CSU CHILL Radar
- S-Band Doppler
- Polarimetric Radar
- Portable Lightning Mapping Array
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Central Oklahoma
- S-band Doppler
- Polarimetric Radar (KOUN)
- Phased Array Radar (PAR)
- SMART-R C-Band
- Doppler
Mobile Radar
- Lightning Mapping Array
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Northern Alabama
- ARMOR Radar –
Doppler & Polarimetric
- Lightning Mapping Array
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Meetings
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Documents
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