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Extinction and optical depths of contrails

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2011
American Geophysical Union Washington, DC

Geophysical research letters 38(11), L11806 () [10.1029/2011GL047189]

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Abstract: One factor limiting the understanding of the climate impact from contrails and aircraft induced cloud modifications is the accurate determination of their optical depth. To this end, 14 contrails were sampled for 2756 s with instruments onboard the research aircraft Falcon during the CONCERT (CONtrail and Cirrus ExpeRimenT) campaign in November 2008. The young (< 10 min old) contrails were produced by 9 commercial aircraft with weights of 47 to 508 t, among them the largest operating passenger aircraft, the Airbus A380. The contrails were observed at temperatures between 214 and 224 K and altitudes between 8.8 and 11.1 km. The measured mean in-contrail relative humidity with respect to ice was 89 +/- 12%. Six contrails were observed in cloud free air, the others were embedded in thin cirrus clouds. The observed contrails exhibited a mean ice water content of 2 mg m(-3) and had a mean number concentration of 117 cm(-3) and effective radius of 2.9 mu m assuming asphericle particles with an aspect ratio of 0.5. Probability density functions of the extinction, with a mean (median) of 1.2 (0.7) km(-1), and of the optical depth tau, with a mean (median) of 0.27 (0.13), are derived from the in situ measurements and are likely representative for young contrails from the present-day commercial aircraft fleet at observation conditions. Radiative transfer estimates using the in-situ measured contrail optical depth lead to a year-2005 estimate of line-shaped contrail radiative forcing of 15.9 mWm(-2) with an uncertainty range of 11.1-47.7 mWm(-2). Citation: Voigt, C., U. Schumann, P. Jessberger, T. Jurkat, A. Petzold, J.-F. Gayet, M. Kramer, T. Thornberry, and D. W. Fahey (2011), Extinction and optical depth of contrails, Geophys. Res. Lett., 38, L11806, doi:10.1029/2011GL047189.

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Note: The CONCERT campaign was organized by the HGF-junior research group AEROTROP (http://www.pa.op.dlr.de/AEROTROP). Part of this work was funded within the DLR-project CATS and by the DFG SPP HALO 1294. We thank the DLR flight department, the Deutsche Lufthansa (A. Waibel) and DFS for excellent support. D. Schauble, T. Hamburger, A. Minikin and J. Gasteiger are thanked for instrument preparation. H. Schlager provided NOy data. We further thank M. Ponater, C. Fromming and R. Rodriguez de Leon for stimulating discussions.

Contributing Institute(s):
  1. Stratosphäre (IEK-7)
Research Program(s):
  1. Atmosphäre und Klima (P23)

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 Record created 2012-11-13, last modified 2024-07-12