banniere  
 
 
 
 
 
Soil Moisture and Ocean Salinity Mission (SMOS)
CBSA

2008 CBSA SMOS OPS preparatory optimisation note. - new
SO-TN-CBSA-SYS-0006-02.a - (31/10/2008)
pdf
CBSA Binding list propagation scheme for preparing ECMWF grib for SML2PP processor -
SO-TN-CBSA-GS-0019 (11/7/2008)
pdf
CBSA SMOS OPS preparatory optimisation note. -
SO-TN-CBSA-SYS-0006-01.b - (28/7/2008)
pdf
2007 CBSA Pixel geometry for a tilted, space borne interferometricRadiometer (SO-TN-CBSA-GS-0016 Issue: 1.a (31/10/2007 ) pdf
  Overall System Performance Synthesis Report
(SO-TN-CESBIO-SYS-1184) - 31/01/2007
pdf
2006 CBSA Algorithm validation plan for SMOS level 2 SMPPD / SO-TN-CBSA-GS-0015 / draft 1.g (09/11/06)
pdf
CBSA Preliminary statistics on SLOS land working areas (4/2006)
pdf
CBSA Impact of the variable angular apodization function on galactic contribution (06/04/2006)
pdf
CBSA Flagging the topographic impact on the SMOS signal (15/03/2006)
pdf
CBSA SMOS L2 processor discrete flexible fine grid definition (1/2006)
pdf
2005 CBSA ECMWF DATA Requirements For level 2 SM processor (7/2005)
pdf
CBSA Approximating the weighting function to be used in the SMOS L2 processor (6/2005) pdf
CBSA Coverage loss due to calibration periods (3/2005) pdf
2004 CBSA SMOS level 2 processor high level requirements (7/2004) pdf
CBSA SMOS Level 3 & 4 data User Model (7/2004) pdf
CBSA Brightness temperature products for browsing (7/2004) pdf
CBSA SMOS geolocation natural targets (9/2004) pdf
CBSA Radiometric biases when using a wide beam radiometer (9/2004) pdf
CBSA Summary note on SMOS calibration issues (3/2004) pdf
CBSA Overall system performance synthesis report (5/2004) pdf
2003 CBSA Note on SMOS calibration and validation (10/2003) (540K) pdf
CBSA Mission products and data processing requirements for SMOS (3/2003) pdf
CBSA Note on suggested archival scheme for SMOS’level 3 and higher (4/2003) pdf


CESBIO contribution to the activities of the "Centre Aval de Traitement et des Données SMOS" (CATDS)

The CATDS (Centre Aval de Traitement et des Données SMOS) is split in three parts :

  • C-PDC Production Center : produce and dissaminate L3/L4 data (l’IFREMER de Brest)
  • C-EC SM Expertise Center dedicated to « Soil Moisture » (CESBIO, Toulouse)
  • C-EC OS Expertise Center dedicated to « ocean  salinity » (IFREMER, Brest )

new downlod CATDS logos

CNES is in charge of the CATDS, this center is dedicated to :

• Product and disseminate SMOS L3/L4 products
• Reprocess SMOS L3/L4 products when necessary
• Develop, test and validate the SMOS L3/L4 processing chains, in close cooperation with the scientific community (improvement of the processing chains)

Interfaces

♦ Data Processing Ground Segment (DPGS) = ESA Center for L1 data production
♦ Users :

• Send services/information requests
• Receive L3/L4 data (network and media) and services

♦Auxiliary data providers, Main auxiliary data provider is the European Centre for Medium-Range Weather Forecasts (ECMWF);
Scientific community : provides expertise with the means provided by the center (C-EC) :

• mock-up (algorithm test)
• specify the "algorithm theoritical baseline document" (ATBD)
• test and evaluation on SMOS data to C-EC

♦ C-PDC / C-EC : expertise and production centers.

Industry implication :

- System architecture : groupement ATOS Origin – GFI Informatique
- Processing chains : consortium CAP-Gemini Sud et ACRI-ST

Cooperations

♦ IFREMER will host the Data Production Centre in the CERSAT (=Centre ERS d'Archivage et de Traitement)

♦ CESBIO will host the SM Expertise Centre; and will deliver the L3+L4 algorithms specifications and mock-up (with the help of the other laboratories involved in L3/L4 SM)

♦IFREMER will host the OS Expertise Centre; and will deliver the L3+L4 algorithms specifications and mock-up (with the help of the other laboratories involved in L3/L4 OS)

♦Spain will develop CP34, another ground-segment dedicated to SMOS L3+L4 products processing

 

 

ATBD

SMOS level 2 Processor for Soil Moisture ATBD (Algorithm Theoretical Based Document) Prepared by the Expert Support Laboratories CESBIO, IPSL-Service d’Aéronomie,INRA-EPHYSE, Reading University, Tor Vergata University For Array Systems Computing Inc. Issue 3.a   Date 05/12/2007 pdf
SMOS level 2 processor Soil moisture ATBD (31/08/2006) pdf
SMOS level 2 processor for soil moisture - Algorithm Theoretical Based Document
(ATBD) - Prepared by the Expert Support Laboratories (15/03/2006)
pdf
Algorithm Theoretical Based Document (ATBD) Date: 15/01/2006 image
SMOS SSS L2 ATBD (Draft issue 4, 3 Oct.. 2005) pdf
Coordinated answer to the scientific contribution to the SMOS soil moisture prototype processor development" Date 29/09/2004 image

 

 

The Living Planet Program Soil Moisture and Ocean Salinity (MIRAS on RAMSES)

 

The SMOS mission was born from the conjonction of new technological developments (CASA EADS et Thales Alenia Space) and the modeling needs for meteorological prediction.

The scientific objective of this mission is to obtain a better estimate of the spatio-temporal water budget at the global scale and ocean/atmosphere interactions.


Proposal in answer to the Call for Earth Explorer Opportunity missions

 L.I. : Yann H. Kerr

CESBIO
(CNRS-CNES-UPS-IRD)

logo ESA
you can visit the SMOS dedicated pages
at the ESA web site
logo_cnesand SMOS pages at the CNES web site

new Have a look at the Microrad call for papers.

            available at the Microrad2010 website
            Thank you for helping to advertise.

 

11th Specialist Meeting on
Microwave Radiometry
and Remote Sensing of the Environment 1-4 March 2010
Washington, DC, USA

 

Dear Colleagues

As SMOS images are starting to float around in a quasi-Brownian way I thought that you were entitled to have a look at what is coming out of this wonderful mission before anyone else. So here are a few pictures, but please remember two things:

1) Those are very preliminary images. They are not calibrated, the reconstruction algorithm is partly running on old, not yet updated, values; we are not sure of the FOV exact limits and so on. This means that they cannot be related to real values whatsoever

2) They are for your eyes only. I would ask you to keep them to yourselves as they are approximate, etc.

Now for some explanations (or should I say pseudo-educated guesses). The image of Madagascar was amongst the very first. The instrument was not even totally regulated at the first phase (10°C).

The one over Alaska down to Mexico is of good quality; so good, in fact, that François even had a go at retrieving soil moisture. Of course, values do not mean much, but do show the algorithm runs.

The global ones over Antarctica and the Arctic also show that it works fine (with all the above-mentioned caveats)! My colleague was flabbergasted to see that the values were close to what he expected!

Finally, the standard global ones show much red for which there are many plausible explanations. Here is my first idea (so probably wrong!): untuned reconstruction algo + poor calibration (e.g., Amazon basin, parts of Australia, parts of Africa), sun somewhere where it should not be? RFI.
Some are quite obvious (southernmost point of Greenland), which also show some smearing effect which could be reduced once the L1 processor has been tuned and finalised with all the necessary data yet to be collected. There are nevertheless some points where a plausible explanation is a little harder to come by and we are all working on this. In the mean time a great many thanks to the teams in Toulouse (LEOP ) and ESAC for their hard work making these pictures available so quickly.

Cheers
Yann

 


 

1st SMOS images

SMOS in-orbit commissioning

SMOS in-orbit commissioning as been on track since the succesful launch of the satellite on November 2nd, 2009.

Following accurate injection, payload arms deployment and fine tuning of the orbit, the first period was dedicated to PROTEUS bus. Full review of platform capability being conducted, after the instrument was switched on on November 17th, 2009, mission commissioning per se was started.

After a full functional health check of all calibration and acquisition modes, instrument characterisation has begun in sequences, each of which yielding an improvement in data quality.

Only concerns have been with one of the local oscillator, which had to be switched to backup side, and with strong presence of RFI over some specific areas.

Current status is that the instrument is behaving better than expected and studies are being initiated to mitigate RFI impact.

For more information, details in real time on the in-orbit are published on the blog: SMOS_blog

 

smos

  Introduction
  Objectives and project status
  Charactéristics and context
  Participants
 
  Activities
  LEWIS
  SMOSREX
  CoSMOS-2
  Processeur Niveau 2
  CAL-VAL
  SMOS in-orbit commissioningnew
  CATDS new
   
  Documents
  ATBD
  CBSA
  SAG
  Technical notes
  Other documents
  SMOS workshops
  Publication List
   
    SMOS simulations
 

Google Earth animation

   
    Images, photos...
  Posters / photos /
  Artist Views / animations new
  newSMOS_blog
from the CESBIO team
  Useful links
   
 
For any questions or comments
on this mission, please contact :
yann.kerr@cesbio.cnes.fr 



© Copyright 2008 CESBIO, 
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