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Forecast Model

We provide a variety of information and common sense related to the space propagation environment.

Radio Blackouts

  • ASSA
    Sunspot

    Detection of Sunspot Groups, Coronal Holes, Filaments

    • SDO HMI, AIA data and ground-based H-alpha data are used
    • Morphological feature detection and estimation of necessary quantitative parameters by various image processing techniques
    • McIntosh and Wilson Magnetic Classification results are automatically generated
    • Update Period: 1 hour
Current

※ Click the image to enlarge.

  • Fig1 Spot group detection and McIntosh classification result[TEXT INFO]

  • Fig1 Spot group detection and McIntosh classification result

  • Fig1 Spot group detection and McIntosh classification result [TEXT INFO]

  • Fig1 Spot group detection and McIntosh classification result [TEXT INFO]

  • PFSS

    Visualization of the sun's open and closed magnetic field lines

    • Macroscopic solar magnetic field numerical model using SDO HMI data
    • Line of sight reconstruction of 3D solar magnetic field
    • Distinguish between open and closed solar fields
    • Update Period: 1 day
Current

※ Click the image to enlarge.

  • Fig1 Spot group detection and McIntosh classification result [TEXT INFO]

  • Fig1 Spot group detection and McIntosh classification result [TEXT INFO]

  • AI기반 신규
    ASSA모델

    Visualization of the sun's open and closed magnetic field lines

    • Macroscopic solar magnetic field numerical model using SDO HMI data
    • Line of sight reconstruction of 3D solar magnetic field
    • Distinguish between open and closed solar fields
    • Update Period: 1 day
Current

※ Click the image to enlarge.

  • Fig1 Spot group detection and McIntosh classification result [TEXT INFO]

  • Fig1 Spot group detection and McIntosh classification result [TEXT INFO]

  • Contact : KSWC, Forecast&Observation, Jaehun Kim (jhkimsip@korea.kr)
  • Developer : SELab, Inc. (jdlee@selab.co.kr)