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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

 

Chris Cantrell
NCAR- ACD
303-497-1479

 

William Brune
PSU
814-865-3286

 

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

 

Don MacGorman
U. of Oklahoma
405-325-5667

 

Laura Pan
NCAR-ACD, TIIMES
303-497-1467

 

Walter Petersen
NASA-MSFC
256-961-7861

 

Kenneth Pickering
NASA-Goddard
301-405-7639

 

Jeffrey Stith
NCAR-EOL
303-497-1032

 

Andy Weinheimer
NCAR-ACD
303-497-1444

 

DC3 Field Experiement logoClick figures to view the details

 

DC3 Experimental Design - January 2009

DC3 Science Plan - January 2009

 

The Deep Convective Clouds and Chemistry (DC3) field campaign will investigate the impact of deep, midlatitude continental convective clouds, including their dynamical, physical, and lightning processes, on upper tropospheric (UT) composition and chemistry. The campaign will make use of extensively instrumented aircraft platforms and ground-based observations.

The NSF/NCAR Gulfstream-V (GV) aircraft is the primary platform to study the high altitude outflow of the storms, and is instrumented to measure a variety of gas-phase species, radiation, and cloud particle characteristics. The GV will also document the downwind chemical evolution of the convective plume.

DC3 Experiment ScopeThe NSF/NCAR C-130 (C-130) aircraft complements the GV via in situ observations to characterize the convective storm inflow and provides remote sensing to aid in flight planning and column characterization.

Ground-based radar networks are used to depict the physical and kinematic characteristics of storms and provide guidance to the aircraft operations. The impact of lightning on outflow composition is constrained through detailed measurements from VHF lightning mapping arrays.

DC3 surpasses previous experiments addressing these topics by using advanced instrumentation not previously available. The DC3 field experiment also includes ground-based collection of precipitation followed by chemical analysis. Satellite data are used to place the airborne and ground-based measurements in the context of the wider geographical region and help guide sampling strategies. At the same time, DC3 measurements help satellite retrievals of atmospheric constituents such as NO2 near storms.

The observations will be conducted in three locations: 1) northeastern Colorado, 2) central Oklahoma, and 3) northern Alabama in order to gather data on different types of storms and with different boundary layer compositions as well as to ensure sampling of convection during the time period of the field campaign. The types of storms being sampled are air mass, multicell, and supercellular convection.




Motivation

Mature airmass thunderstorm & squall line cross section

Schematic of a) a mature airmass thunderstorm and b) a squall line vertical cross section. Taken from the NOAA National Weather Service http://www.srh.weather.gov/srh/jetstream/index.htm. Superimposed on panel b are processes affecting chemical species that are ingested into storms.

The upper troposphere and lower stratosphere (UTLS) is an important region for Earth’s climate because water vapor, ozone, cirrus clouds and aerosols in this region strongly contribute to radiative forcing of the climate system.

The UT and LS have very different chemical compositions resulting in strong gradients across the tropopause. Further, the UTLS is a highly dynamic region influenced by a broad range of scales, from deep convection and gravity waves, to tropospheric weather systems and the stratospheric large-scale circulation.

Convective transport is a major pathway for rapidly moving chemical constituents and water from the boundary layer to the upper troposphere and in some cases to the lower stratosphere. Yet the impact of convective transport on the UTLS composition and chemistry has not been fully characterized on either the global or continental scale.

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.

DC3 is proposed to study the impact of continental, midlatitude deep convection on the UTLS composition and chemistry above the continental U.S. during the lifetime of the storm itself and during the period 12-48 hours after active convection.

 

DC3 will give us:
  • Comprehensive chemistry on board a high-altitude and lower-altitude aircraft.  The NSF/NCAR HIAPER and C-130 are being requested.

  • Comprehensive storm information from ground-based Doppler and polarimetric radars

  • Outstanding information on lightning location from lightning mapping arrays



Science Goals

AnvilTo quantify and characterize the convection and convective transport within the first few hours of active convection, investigating:
  • storm dynamics and physics,

  • lightning and its production of nitrogen oxides,

  • cloud hydrometeor effects on wet scavenging of species,

  • chemistry in the anvil

To quantify the changes in chemistry and composition after active convection, focusing on
  • 12-48 hours after convection and

  • the seasonal transition of the chemical composition of the upper troposphere

 


Ancillary Goals

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

  • To characterize aerosols in the thunderstorm environment





Experimental Design

- DC3 Experimental Design - January 2009
- Platform & Payload Information - January 2009


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. NSF/NCAR C-130 or 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 and utilize (existing) ground based networks to sample in diverse precipitation, lightning and background chemistry regimes:

LMA
Northeast Colorado

Operated by Colorado State University

  • CSU-CHILL Radar
  • Pawnee national radar facilities
Precipitation
S-Band Doppler & Polarimetric radar (KOUN) & Phased Array Radar (PAR)
Central Oklahoma

Surface facilities maintained by the National Severe Strom Laboratory & University of Oklahoma

 

 

  • SMART-Rs C-Band
  • KOUN polarimetric radar
  • Oklahoma Lightning Mapping Array
ARMOR RadarNorthern Alabama

Facilities operated by the University of Alabama-Huntsville & NASA Marshall Space Flight Center

  • ARMOR polarimetric radar
  • MAX X-band radar
  • Northern Alabama lightning mapping array
  • MIPS moblile sounding facility

Forecasting:

Forecasting for DC3 operations will be accomplished through the use of guidance from both operational and research numerical models.


Satellite Data:

Satellite Data will be used to examine the influence of convection on the UTLS composition and chemistry. These spaceborne data will be used before the DC3 field deployment to better prepare for the operating period.


Post-Mission Numerical Modeling & Analysis:

Post-mission modeling efforts will include cloud-resolving numerical models and model that utilize parameterized convection (e.g., regional models).

 


Meetings

DC-3 Planning Workshop

12 - 13 August 2008

NCAR, Foothills Lab Main Auditorium

 

Goals: 

  • Finalize the Scientific Objectives & complete planning on the experimental design.
  • Incorporate science of new investigators if there are any. 
  • Set plans to finalize the SOD and EDO documents.
  • Decide if an additional briefing at NSF is necessary. 
  • Discuss NASA DC-8 involvement especially if a formal proposal is needed.


Documents