WBMOD Ionospheric Scintillation Model

This program provides estimates of the effects of ionospheric scintillation on the transionospheric radio channel for frequencies above 100 MHz. It is based on a climatology of F-region electron-density irregularities that cause scintillation (Secan et al. 1995, 1997) and a power-law, phase-screen propagation model (Rino, 1979). The model is global, and includes variations with solar cycle, season, geomagnetic disturbance levels, and local time. Further information can be found at the WBMOD model WWW site.

Contributor(s)
Initial contribute: 2019-07-02

Authorship

  • E. J. Fremouw, J. A. Secan
    • :  
    Northwest Research Associates, Inc.
    :  
    scint@nwra.com
    Is authorship not correct? Feed back

    Classification(s)

    ● Application-focused categoriesNatural-perspectiveSpace-earth regions

    Detailed Description

    English {{currentDetailLanguage}} English

    Quoted from: https://ccmc.gsfc.nasa.gov/modelweb/ionos/wbmod.html

    Parameter: Ionospheric scintillation effects

    Brief Description:
    This program provides estimates of the effects of ionospheric scintillation on the transionospheric radio channel for frequencies above 100 MHz. It is based on a climatology of F-region electron-density irregularities that cause scintillation (Secan et al. 1995, 1997) and a power-law, phase-screen propagation model (Rino, 1979). The model is global, and includes variations with solar cycle, season, geomagnetic disturbance levels, and local time.
    Further information can be found at the WBMOD model WWW site.

    Availability: Contact authors for release information.

    References:
    Fremouw, E. J., and J. A. Secan, Modeling and scientific application of scintillation results, Radio Sci., 19, 687-0694, 1984.

    Fremouw, E. J., and A. Ishimaru, Intensity scintillation index and mean apparent radar cross section onmonostatic and bistatic paths, Radio Sci., 27, 539-543, 1992.

    Rino, C. L., A power law phase screen model for ionospheric scintillation, 1, Weak scatter, Radio Sci., 6, 1135-1145, 1979.

    Secan, J. A., R. M. Bussey, E. J. Fremouw, and Sa. Basu, An improved model of equatorial scintillation, Radio Sci., 30, 607-617, 1995.

     

    Secan, J. A., R. M. Bussey, E. J. Fremouw, and Sa. Basu, High-latitude upgrade to the Wideband ionospheric scintillation model, Radio Sci., 32, 1567-1574, 1997.

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    模型元数据

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    E. J. Fremouw, J. A. Secan (2019). WBMOD Ionospheric Scintillation Model, Model Item, OpenGMS, https://geomodeling.njnu.edu.cn/modelItem/57ee7f85-8aad-452f-868a-9974d72a0f18
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    Contributor(s)
    Initial contribute : 2019-07-02

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    Authorship

  • E. J. Fremouw, J. A. Secan
    • :  
    Northwest Research Associates, Inc.
    :  
    scint@nwra.com
    Is authorship not correct? Feed back

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