smos+ storm evolution kick-off meeting, 2 april 2014 solab work description zabolotskikh e.,...

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SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014 SOLab work description Zabolotskikh E., Kudryavtsev V.

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SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

SOLab work description Zabolotskikh E., Kudryavtsev V.

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

Rational

• Contribution to WP1100: L-band Signal Response over the Ocean in very high wind speed conditions (with the focus on model analysis on the potential effect of rain in TC & storms on the L-band microwave brightness over the ocean);

• Contribution to WP1400: Merged Multi-mission Wind Speed product Algorithm (AMSR2 wind speed retrievals under rain in hurricanes) and WP2000: Generate & Validate SMOS High Wind Speed Product Databases;

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

1) Rain increases the atmospheric attenuation, especially at higher frequencies. Therefore under rain the radiometer measurement is less sensitive to the surface wind speed;

2) It is very difficult to accurately model brightness temperatures in rain due high variability of rainy atmospheres (dependency on liquid drop form and size distribution, start of scattering);

3) The brightness temperature signals of rain and wind are very similar. Therefore the rain free wind speed algorithm tends to treat an increase in rain the same way as an increase in wind speed;

4) Intensive rain also changes the ocean surface and its properties and this effect is mostly hard to be studied (separated from atmospheric or wind influence);

Rain impact on microwave brightness temperature

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

1) Select the RTM to be used in the analysis and code it (RTM without rain is established at SOLab, rain module should be incorporated;

2) Conduct RTM simulations and estimate the expected observational dependencies (in terms of incidence angle, polarization, radiometer footprint) of Tb on rain rate;

Study of potential effect of rain in TC & storms on the L-band microwave brightness

7 October 2013

TRMM Radar

TRMM TMI

RRmax=150 mm/h

RRmax=15 mm/h

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

On 18 May 2012 Japan launched a new passive microwave instrument with the largest in the world diameter of antenna - Advanced Microwave Scanning Radiometer (AMSR2) onboard Global Change Observation Mission – Water satellite (GCOM-W1 “Shizuku”)

Additional channel Better than AMSR-E

Same as AMSR-EPotential accuracy for SWS retrievals is 1 m/s

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

AMSR2 rain free wind speed retrieval algorithms

• Are based on numerical experiment and physical modeling of AMSR2 brightness temperatures;

• Use Neural Networks as an inversion function;

• Are validated using Norwegian and North Sea oil platform high wind speed measurements;

• Two SWS algorithms are developed – 1) using low frequency AMSR2 channels (LF algorithm - higher accuracy, lower resolution) and 2) using higher frequency AMSR2 channels (HF algorithm - lower accuracy under optically thick atmospheres, higher resolution);

• Use newly developed atmospheric filtering based on the value of total atmospheric absorption 10.65 as a criterion for weather masking;

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

AMSR2 SWS Surface wind speed (SWS) in the extratropical cyclone 29 January 2013

AMSR2 JAXA standard product AMSR2 new algorithm

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

Development of AMSR2 all weather wind speed retrieval algorithms

Brightness temperature fields measured by AMSR2 on 7 November 2013 at 4:20 UTC over the typhoon Haiyan (a) at 10.65 GHz, vertical polarization and (b) at 89 GHz, vertical polarization and (c) Aqua MODIS visible image at 4:23 UTC . Area A, marked by dark green line, corresponds to rain-free region. The black dot corresponds to the typhoon center

A A A

a b c

• Atmospheric parameter variations influencing TB in C- and X-bands are negligible for the area of equal distance from the cyclone center which does not relate rain (A section);

• Though wind speed variations influencing TB in C- and X-bands cannot be priori considered negligible (wind field can be significantly asymmetric), wind dependency in C- and X-bands is very similar. So to some extension TB V

7,6 = TB 7.3V-TB 6.9

V and TB V10,7 = TB 10.65

V-TB 7.3V do not

depend on the sea state but rather the functions of rain rate;

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

over most rainy atmospheres rain radiation at 10.65, 7.3, and 6.9 GHz can be parameterized in terms of TBV

7,6 and TBV10,7. and related to rain

rate (RR). After subtraction of the rain part from the total TB rain-free SWS can be applied.

General idea

(a) TMI rain rate field (mm/h) for the typhoon Danas on 7 October 2013 (http://www.remss.com/) at 18:36 UTC; (b). AMSR2 derived rain brightness temperature (K) at 10.65 GHz vertical polarization at 17:14 UTC. White dots indicate the center of the typhoon at 17:14 UTC

a b

SMOS+ STORM Evolution Kick-off Meeting, 2 April 2014

Work plan:

• Parameterize the rain part of the microwave radiation over TC & storms for AMSR2 channels (C and X-bands) as a function of TB 7.3

V-TB 6.9V and TB 10.65

V-TB7.3V ;

• Develop an algorithm for Rain Rate retrieval from AMSR2;

• Develop the methodology for RFI area detection for the channels used in the algorithms;

• Validate RR algorithm using TMI RR (create a collocated data set);

• Process AMSR2 data for TC events starting from August 2012 (generating AMSR2 SWS and RR products);