Presentation based on paper: M. E. Gorbunov, A. V. Shmakov, S. S. Leroy, K. B. Lauritsen,

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OPAC-2010 1 Presentation based on paper: M. E. Gorbunov, A. V. Shmakov, S. S. Leroy, K. B. Lauritsen, Submitted to J. Atm. Ocean. Tech. (2010) Processing of COSMIC radio occultation data and cross-center comparison K. B. Lauritsen (DMI), M. E. Gorbunov (IAP), S. S. Leroy (HSEAS), A. V. Shmakov (IAP)

description

Processing of COSMIC radio occultation data and cross-center comparison. K. B. Lauritsen (DMI), M. E. Gorbunov (IAP), S. S. Leroy (HSEAS), A. V. Shmakov (IAP). Presentation based on paper: M. E. Gorbunov, A. V. Shmakov, S. S. Leroy, K. B. Lauritsen, Submitted to J. Atm. Ocean. Tech. (2010). - PowerPoint PPT Presentation

Transcript of Presentation based on paper: M. E. Gorbunov, A. V. Shmakov, S. S. Leroy, K. B. Lauritsen,

Page 1: Presentation based on paper: M. E. Gorbunov, A. V. Shmakov, S. S. Leroy, K. B. Lauritsen,

OPAC-2010 1

Presentation based on paper:M. E. Gorbunov, A. V. Shmakov, S. S. Leroy, K. B. Lauritsen,Submitted to J. Atm. Ocean. Tech. (2010)

Processing of COSMIC radio occultation data and cross-center comparison

K. B. Lauritsen (DMI), M. E. Gorbunov (IAP),S. S. Leroy (HSEAS), A. V. Shmakov (IAP)

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Processed COSMIC data:- 20 days from each of the years 2007, 2008, 2009 (from 2009: data version 2009.2650 starting April 1);

Processing of atmPhs files with OCC (similar to GRAS SAF ROPP_PP software);

Results are compared to:

- UCAR processed data: atmPrf files (refractivities);

- ECMWF analyses (refractivities);

COSMIC data & ECMWF fields

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State of the art Fourier integral operator code (CT2) ensures high accuracy (GO used above 25 km)

SO: optimal linear combination based on initialization to ECMWF or 2-parameter fitted MSIS climatology

Quality control based on L2-signal and SO-solution: Q = QL2 + QSO

Cutoff of u(t): at SLTA = -250 km

Radio-holographic (RH) filtering:

- phase: no; CT-amplitude: yes

- full RH filtering results in positive bias from suppression of large BAs and MP structures in wide-band signal tails [Sokolovskiy, 2009]

OCC processing and options

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OCC 2009: #occ

About half the profiles penetratedown to 1 km

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OCC-ECMWF: 2007 REF

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OCC-ECMWF: 2008 REF

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OCC-ECMWF: 2009 REF

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OCC-UCAR: 2009 REF

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Zoom on tropical bias, 2009 data

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Tropics (0-300), with RH-filtering

RH filtering:

phase: yes

CT-amplitude: yes

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Tropics (0-300), with no RH-filtering

RH filtering:

phase: no

CT-amplitude: no

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Cutoff at SLTA = -150 km

RH filtering: phase: yes

2-parameter MSIS fit

OCC-UCAR: 2009 REF, alternative options

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Cutoff at SLTA = -250 km

RH filtering: phase: no

Initialization to ECMWF

OCC-UCAR: 2009 REF, optimal options

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OCC-ECMWF differences : 2007, 2008, 2009Change in ECMWF cycle 32r3 in 2008: i) COSMIC RO assimilated to surface ii) updated convection and entrainment physics

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OCC-UCAR: 2009 raw BA

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OCC-UCAR: 2009 Tdry

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Results

Comparison of OCC and UCAR refractivities for three different years (2007, 2008, 2009)

Tropics:

- relative difference is smaller than 0.1% for 2-30 km (and smaller than 0.03% for 9-25 km)

- 0.2% bias below 1 km, due to different cutoff and filtering

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