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Traceability and consistency of COSMIC radio occultation in comparison with NOAA-20 CrIS infrared sounder observations



Details

  • Journal Title:
    Earth Observing Missions and Sensors: Development, Implementation, and Characterization V
  • Personal Author:
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  • Description:
    The Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) satellite system for the Radio Occultation (RO) mission provides advances in meteorology, ionospheric research, climatology, and space weather by utilizing the readily available Global Navigation Satellite System (GNSS) signals in conjunction with GNSS receivers in low Earth orbiting (LEO) satellites. COSMIC was launched in 2006 with six satellites in a constellation known as FORMOSAT-3 in low inclination orbits to provide global coverage. RO relies on the calculation of GNSS signal time delay in carrier phase due to the atmosphere in the L1 and L2 signals transmitted between the GNSS and receiving satellites in the LEO orbit, from which the bending angle, refractivity, and atmospheric profiles can be retrieved. Since the Atomic Frequency Standard (AFS) based GNSS signal is International System of Units (SI) traceable, is actively maintained, and the precise orbit of both the GNSS and the LEO satellites can be determined accurately, RO data from COSMIC have been recognized as stable references for data assimilation (DA) in Numerical Weather Prediction (NWP) models. Currently, NWP customers are eager to obtain similar data from COSMIC2 which will be launched in the next few months to mitigate the aging COSMIC constellation and diminishing number of ROs.
  • Source:
    Earth Observing Missions and Sensors: Development, Implementation, and Characterization V, 119, 31
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    Other
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    Library
  • Main Document Checksum:
    urn:sha-512:0698b52f9539441c58bb9ab1f93f076976be2e971fb1f1bdd87578578d419a776444f65e31766b8ec721334bd5904e193b95057d1a1aa46e995fc5e6c5b97982
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