HALO-South

The interplay of Clouds, Aerosols and Radiation above the Southern Ocean
Mission status: Completed.
Persons in Charge
Mission-PI
- Mira Pöhlker, Leibniz Institute for Tropospheric Research (TROPOS), Leipzig
Mission coordinator
- Stephan Mertes, Leibniz Institute for Tropospheric Research (TROPOS), Leipzig
Contact point at DLR-FX for this mission:
- Andreas Minikin (HALO Project Management): +49 (0)8153 28-2538 (office), +49 (0)174 9511618 (mobile), : andreas [dot] minikin [at] dlr [dot] de
HALO Deployment Base
Time Period
July – October 2025
Mission phases
- 02 Jul 25 – 29 Aug 25 || Preparation, Payload integration, EMI testing
- 01 Sep 25 – 17 Oct 25 || Mission execution
- 20 Oct 25 – 23 Oct 25 || Dismounting of Payload
Project description
The Southern Ocean is one of the cloudiest regions on earth with a high cloud radiative effect, with a high bias in atmospheric models. However, observations have shown that clouds over the Souther Ocean amplify the warming in this region.
It is also one of the few regions on earth with frequent pristine aerosol conditions where the effect of aerosols on clouds is biggest. The source of Cloud Condensation Nuclei in pristine oceanic regions is expected to be coupled to clouds and appears in the upper troposphere. The HALO-South mission is planned to take place in the Southern Ocean region mainly south-west and south of Christchurch, New Zeeland, from September to October 2025. This will be at the end of the winter and the onset of the spring in the Souther Ocean. The HALO aircraft is equipped with a unique set of instrumentation to investigate aerosol and cloud cycles and its effect on radiative properties of the clouds. The campaign will be embedded in parallel intensive field activities including ground-based measurements from New Zeeland and will be supported by satellite investigations. HALO-South will provide pressing knowledge about the relation between aerosols and clouds in the southern hemisphere from cloud droplet and ice nucleation to the production of cloud and ice active particles partly triggered by increased radiation above clouds and cloud optical properties. These findings will be extrapolated to a larger scale using satellite data and global climate models. The campaign will greatly build on and continue past HALO campaigns with focus on either cloud and aerosol or gas and aerosol properties (CIRRUS-HL, ACRIDICON, CAFE-Pacific, CAFE-EU, CAFE-Brazil, CAFE-Pacific and will also overlap with EMeRGe-EU and EMeRGe-Asia). This campaign will cover the full cycle to study aerosols through clouds and the full cycle of clouds with a particular focus on mixed-phase clouds, as this is where we expect the important microphysical processes affecting aerosols and radiation to take place.
Partners
- Leibniz Institute for Tropospheric Research (TROPOS)
- Leipzig University, Leipzig Institute for Meteorology (LIM)
- Johannes Gutenberg University Mainz (JGU)
- Goethe University Frankfurt (GUF)
- Max Planck Institute for Chemistry (MPIC), Mainz
- Karlsruhe Institute of Technology (KIT)
- German Aerospace Center, Institute of Atmospheric Physics (DLR-IPA)
- Forschungszentrum Jülich (FZ Jülich)
Scientific instruments and payload configuration
List of scientific instruments for the mission:
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SMART-Albedometer
spectral radiance, spectral irradiance l= 350–2200 nm | M. Wendisch (Uni Leipzig)
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BACARDI
broadband upward and downward irradiances | A. Giez (DLR-FX) & M. Wendisch (U. Leipzig)
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HALO-SR
pectral actinic flux densities 280-660 nm | B. Bohn (FZJ) & M. Wendisch (U. Leipzig)
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AENEAS
NO, NOy | H. Ziereis (DLR-PA)
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AMTEX-2C
CO, O3, CH4 | H. Ziereis (DLR-PA)
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FASD
aerosol number and size distribution, including nucleation mode particles 1.5 nm to 5 μm | M. Pöhlker (TROPOS)
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Aerosol Rack Insert
aerosol size distribution (10-30 nm), volatility of particles & optical properties | D. Sauer (DLR-PA)
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SOPAMA
Refractive black carbon (rBC) particle mass and absorption coefficients at 3 wavelengths | D. Sauer (DLR-PA)
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C-ToF-AMS
bulk aerosol composition (non-refractory) | J. Schneider (MPI-C)
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ALABAMA
single particle chemical composition of aerosol / cloud residuals > 150 nm | J. Schneider (MPI-C)
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CCN-Rack
cloud condensation nuclei (CCN) number concentration, reflective black carbon (BC) properties, aerosol impactor | Y. Cheng (MPI-C) & U. Pöschl (MPI-C)
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HALO-CVI
cloud particle residual number (> 10 nm), size distribution (60 – 1000 nm), and absorption coefficient, cloud water content | S. Mertens (TROPOS)
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miniCCNC
fast scanning cloud condensation nuclei (CCN) | F. Stratmann (TROPOS)
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Hear4HALO
high temperature Ice nucleating particle number concentration (INP) | F. Stratmann (TROPOS)
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PINEair
INP and temperature spectrum at low temperature | J. Curtius (GUF Frankfurt) & O. Möhler (KIT)
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PCASP-100X
Aerosol size distribution, 0.12-3.5 μm | D. Sauer (DLR-PA)
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NIXE-CAPS
Particle size distribution, polarization, 0.6-50 μm | C. Voigt (DLR-PA/JGU Mainz)
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CCP (CDP/CIP)
particle size distribution, shape CDP 3-50 μm; CIP 15-960 μm | C. Voigt (DLR-PA / JGU Mainz)
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PIP
particle size distribution, shape, 100-6400 μm | C. Voigt (DLR-PA / JGU Mainz)
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BCPD
backscatter cloud probe with depolarization detection | C. Voigt (DLR-PA / JGU Mainz)
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PHIPS-HALO
light scattering, polarization, particle size distribution, 10-1000 μm | M. Pöhlker (contact person; MPI-C)
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BAHAMAS
P, T, wind, humidity, TAS, position, alt. | A. Gierz (DLR-FX)
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SHARC
H2O mixing ratio (gas phase) | A. Giez (DLR-FX)
Cabin and exterior configuration of HALO for the mission
HALO flights for this mission
Flights are listed by
Aircraft registration | Date | Take-off / Landing (UT) | Total flight time (h) | From / To | Mission #
- D-ADLR | yyyy-mm-dd | hh:mm:ss – hh:mm:ss | h.hh | CODE – CODE | RF01
More information
HALO-South in person Meeting: 28/29 January 2025, Science Park Leipzig (near TROPOS), Leipzig
For information please contact Stephan Mertes (mertes[at]tropos.de).
>> Overview of the HALO South mission on TROPOS webpage
>> Overview of the HALO south mission on MPI-C webpage