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    Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/102222


    Title: Ionospheric assimilation of radio occultation and ground-based GPS data using non-stationary background model error covariance
    Authors: 劉正彥;Lin, C. Y.;Matsuo, T.;Liu, J. Y.;Lin, C. H.;Tsai, H. F.;Araujo-Pradere, E. A.
    Contributors: 地球科學學院太空科學與工程學系
    Keywords: Analysis;Computer simulation;Correlation;Correlation analysis;Covariance;Data;Data assimilation;Data collection;Density;Density distribution;Density profiles;Distribution;Electron density;Electron density profiles;Electrons;Empirical analysis;Empirical orthogonal functions;Global Positioning System;Global positioning systems;GPS;Ground-based observation;Incoherent scatter radar;Ionosphere;Ionospheric electron density;Ionospheric models;Kalman filters;Markov chains;Orthogonal functions;Radar;Radar data;Radio;Radio occultation;Total Electron Content
    Date: 2015-01-12
    Issue Date: 2026-04-23 11:04:25 (UTC+8)
    Publisher: Copernicus Gesellschaft mbH;Katlenburg-Lindau: Copernicus Publications
    Abstract: 摘要: Ionospheric data assimilation is a powerful approach to reconstruct the 3-D distribution of the ionospheric electron density from various types of observations. We present a data assimilation model for the ionosphere, based on the Gauss–Markov Kalman filter with the International Reference Ionosphere (IRI) as the background model, to assimilate two different types of slant total electron content (TEC) observations from ground-based GPS and space-based FORMOSAT-3/COSMIC (F3/C) radio occultation. Covariance models for the background model error and observational error play important roles in data assimilation. The objective of this study is to investigate impacts of stationary (location-independent) and non-stationary (location-dependent) classes of the background model error covariance on the quality of assimilation analyses. Location-dependent correlations are modeled using empirical orthogonal functions computed from an ensemble of the IRI outputs, while location-independent correlations are modeled using a Gaussian function. Observing system simulation experiments suggest that assimilation of slant TEC data facilitated by the location-dependent background model error covariance yields considerably higher quality assimilation analyses. Results from assimilation of real ground-based GPS and F3/C radio occultation observations over the continental United States are presented as TEC and electron density profiles. Validation with the Millstone Hill incoherent scatter radar data and comparison with the Abel inversion results are also presented. Our new ionospheric data assimilation model that employs the location-dependent background model error covariance outperforms the earlier assimilation model with the location-independent background model error covariance, and can reconstruct the 3-D ionospheric electron density distribution satisfactorily from both ground- and space-based GPS observations.
    出版者: Katlenburg-Lindau: Copernicus Publications
    出版日期: 2015-01-12
    出處: Atmospheric Measurement Techniques, 2015-01, Vol.8 (1), p.171-182
    資源來源: Publicly Available Content Database
    版權: COPYRIGHT 2015 Copernicus GmbH
    版權: Copyright Copernicus GmbH 2015
    識別號: ISSN: 1867-8548
    識別號: ISSN: 1867-1381
    識別號: EISSN: 1867-8548
    識別號: DOI: 10.5194/amt-8-171-2015
    Appears in Collections:[DEPARTMENT OF SPACE SCIENCE AND ENGINEERING] journal & Dissertation

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