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UTLS - Science - DC3 Field Campaign




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Deep Convective Clouds & Chemistry

Experiment (DC3)

Overview & Goals Instrumentation Meetings & Workshops Documents

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

 
DC3 Experiment Scope

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.




Motivation

UTLS Scope

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



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
  • Can we locate the source of NO within the storm in relation to the kinematics, and the location of the lightning and microphysical structure?

  • Can we determine the production of NOx from intracloud lightning in relation to that from cloud-to-ground lightning?

  • Can we accurately represent all processes affecting constituents?

  • Do the results vary depending on the type of convection

 
AnvilDetermine the mass fluxes of air and trace gases into and out of the storm, including entrainment from the boundary layer, mid-troposphere, and stratosphere
  • What fraction of the boundary layer air reaches the upper troposphere?

  • What’s the degree of entrainment?

  • What part of the boundary layer is ingested into the storm?

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
  • In the anvil, does the scattering of actinic fluxes significantly affect concentrations?

  • What role does adsorption of gases onto ice play in affecting the chemistry?

  • What chemical aging occurs in the convective outflow? Is O3 produced (and how much)?

Contrast the influence of different surface emission rates on the composition of convective outflow
  • Is more O3 produced in convective outflow when the convection occurs over relatively clean regions?

  • What is the importance of biogenic hydrocarbons (e.g. isoprene) on the chemical aging in convective outflow regions?




Ancillary Goals

Lightning Map
  • To improve our understanding of cloud electrification and lightning discharge processes (in relation to NO production; contrasting differences among different convective regimes)

  • 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

  • To connect aerosol and cloud droplet and ice particle number concentrations with convection characteristics and trace gas convective processing

  • To determine partitioning of reactive halogen and reservoir species in the UTLS




Experimental Design

G-V (Hiaper)
High Altitude Aircraft

(e.g. NSF/NCAR G-V) outfitted with gas-phase and aerosol characterization instrumentation to sample convective outflow

 
NASA's DC8
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

 
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:

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



Meetings




Documents