heinemann lidar weddell sea - polar...

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A study of the atmospheric boundary layer in the Weddell Sea using a wind lidar Günther Heinemann, Rolf Zentek Environmental Meteorology, University of Trier, Germany SPP 1158 Antarktisforschung Grants: DFG HE 2740/19 Polarstern AWI_PS96_03 Verification data for atmospheric models radiosondes and observations from Polarstern boundary layer measurements using a wind lidar AWI (2016) Heinemann 2016 Polarstern cruise PS96: 6 Dec. 2015 – 14 Feb. 2016 LIDAR Scanning Doppler wind lidar “Halo-Photonics Streamline“ scanning wind lidar - wavelength 1.5 μm - pulse rate of 15 kHz - eye-safe (class 1m) - resolution 0.038 m/s - accuracy 0.1 m/s (depending on SNR) - band width 19.4 m/s - 18m gates (6x3), overl. High-resolution boundary layer measurements: Profiles, stares and RHI scans (range up to 10km) of wind, turbulence, aerosols

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  • A study of the atmospheric boundary layer in the Weddell Sea using a wind lidar

    Günther Heinemann, Rolf ZentekEnvironmental Meteorology, University of Trier,

    Germany

    SPP 1158Antarktisforschung

    Grants:DFG HE 2740/19 Polarstern AWI_PS96_03

    Verification data for atmospheric models‐ radiosondes and observations from Polarstern‐ boundary layer measurements using a wind lidar

    AWI (2016)

    Heinemann 2016

    Polarstern cruise PS96: 6 Dec. 2015 – 14 Feb. 2016

    LIDAR

    Scanning Doppler wind lidar

    “Halo-Photonics Streamline“ scanning wind lidar- wavelength 1.5 μm- pulse rate of 15 kHz- eye-safe (class 1m)- resolution 0.038 m/s- accuracy 0.1 m/s

    (depending on SNR)- band width 19.4 m/s- 18m gates (6x3), overl.

    High-resolution boundary layer measurements: Profiles, stares and RHI scans (range up to 10km) of wind, turbulence, aerosols

  • Scanning patternsDual stare, triple stare

    windVR

    VR

    VRV

    V

    North or reference direction (ship heading)VR = radial (line of sight LOS) wind) 

    Scanning patterns: Dual stare

    windVR

    VR

    V

    α1

    r V r cos β r α1Horizontal windWind speed V, direction

    tan r α2 α1α1 r α2

    r V r cos β r α2

    α2r

    V r cos β r α1ship heading

    Moving ship dual stare

    windV

    Equivalent to a two‐lidar system observing the same volumewithin a few minutes

    Scanning patterns: RHIDual RHI

    windVR

    V

    r

    z VR r,θ VH,R r,z cos θ

    θ

    VH,R r,z V r,z cos β r,z α1

  • Scanning patterns: VAD

    windV

    z

    8 beams with constant zenith angle θ (15°)

    Wind data processing

    VR = radial (line of sight LOS) wind) 

    Correction for ship heading and velocity

    Ship roll and pitch angles (1Hz)

    Ship time server (1Hz)

    LIDAR INS/GPS (10Hz (‐400Hz))

    Roll, pitch

    LIDAR beams VR(1Hz)

    Roll/pitch‐corrected LIDAR 

    beams VR

    Wind vector relative to the ship’s heading

    radial wind 28 Dec. 1500 UTC

    triple staretriple RHI280, 255, 23510 repeats

    0‐403 repeats

    6s averages

    Turbulence Ronne polynya

    dual stare 280, 255, 30 repeats

    radial wind 13 Jan. 2016, 0800 UTC

    2s averages60 seconds 60 seconds

    Fast ice edge Lee of the ship

    13 Jan. 2016, 0930 UTC

    ‐17°C5‐6m/s

    0, 35 deg

  • A23A 17 Jan20160910 UTC

    © Umweltmeteorologie Universität Trier

    50 km

    Iceberg A23A Lidar

    Station 1

    Station 2

    Station 3

    Start

    Iceberg A23A

    10 m/s

    LLJLLJ

    VAD 17 Jan. 2016

  • Station 2 RHI

    SummaryBetween 23 December 2015 and 30 January 2016: Vertical wind profiles (VAD) scans every 10‐15min, at lot of RHI scans and stares 2‐3 radiosondes per day

    First time of wind lidar measurements on a ship in the Antarctic

    Atmospheric model: COSMO‐CLMCCLM‐15km simulations for 2002‐2015 (ERA‐I)

    In progress:CCLM‐15km Jan.2016

    CCLM‐5km2002‐2016

    Planned:CCLM‐1kmDec. 2015 –Jan.2016

    Ebner et al. (2014) 

    Sea ice / oceanmodel FESOM (down to 3km)

  • Heinemann 2016

    Melt ponds Weddell Sea