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Multi-snapshot inversion of interferometric synthetic aperture microwave radiometry observations for remote sensing

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  • معلومة اضافية
    • Contributors:
      CB - Centre Borelli - UMR 9010 (CB); Service de Santé des Armées-Institut National de la Santé et de la Recherche Médicale (INSERM)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS)-Ecole Normale Supérieure Paris-Saclay (ENS Paris Saclay)-Université Paris Cité (UPCité); Centre d'études spatiales de la biosphère (CESBIO); Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3); Communauté d'universités et établissements de Toulouse (Comue de Toulouse)-Communauté d'universités et établissements de Toulouse (Comue de Toulouse)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE)
    • بيانات النشر:
      CCSD
      IEEE
    • الموضوع:
      2023
    • Collection:
      Archive ouverte du Service de Santé des Armées (HAL)
    • الموضوع:
    • نبذة مختصرة :
      International audience ; The Soil Moisture and Ocean Salinity (SMOS) satellite [3] produces images of L-band brightness temperature using interferometry. The brightness temperatures that gave rise to a set of observed visibilities are inferred by solving an inverse problem based on the Van Cittert-Zernike theorem. The images are generated from visibilities one correlation period at a time, even though a given patch of Earth's surface may be visible to the satellite for 100 consecutive periods. The recovered brightness temperature images are noisy and, due to the antenna array's undersampling of the u-v frequency plane, aliased. A simultaneous inversion of multiple snapshots (call it "satellite-rotation synthesis" or a "global inversion") could take advantage of these multiple looks to improve resolution, field of view, and noise level, but appeared prohibitively expensive computationally and ill-posed: due to directional emissivity, many brightness temperatures must be recovered for each pixel. However, this directional emissivity can be sparsely modeled; accordingly, for satellites like SMOS, the observation model becomes shift-invariant across an orbital segment when expressed in geodetic coordinates relative to the trace. The observation model performs a convolution on the image of parameters (uniform in geodetic coordinates) governing observed brightness as a function of satellite position, and we can use the "Fourier transform trick" introduced in [6], to enable a global inversion. For a future L-band mission, such as the proposed L-Band Interferometer for Fluxes and Interfaces in the Environment (LIIFE) [7], [11], we present a realistic global inversion of the observation model across the orbital trace, which simultaneously unfolds and denoises the aliased snapshots. By using sparse spline models of the brightness temperature parameters, we can ensure this inversion is accurate and stable, even with a realistic simulation that accounts for the difficulty of modeling the Van Cittert-Zernike theorem ...
    • الرقم المعرف:
      10.1109/CAMA57522.2023.10352689
    • الدخول الالكتروني :
      https://hal.science/hal-04473824
      https://hal.science/hal-04473824v1/document
      https://hal.science/hal-04473824v1/file/paper23.pdf
      https://doi.org/10.1109/CAMA57522.2023.10352689
    • Rights:
      http://creativecommons.org/licenses/by/ ; info:eu-repo/semantics/OpenAccess
    • الرقم المعرف:
      edsbas.AC94FF07