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  • SWSM
  • Monitoring synoptic variation of solar wind using IPS data

    Monitoring variation of solar wind velocity and density on the solar surface based on IPS data during 1 Carrington Rotation(about 27 days) which is a standard period of solar rotation

    Based on ground-based STEL, Japan and KSWC, Korea IPS observation

    Developed by the Center for Astrophysics and Space Sciences, UCSD, U.S.A

    Visualizing the distribution of velocity and density of solar wind by updating daily data

    Updating period : 4 hours.

  • Monitoring synoptic variation of the solar wind

  • Fig1. Density
    Fig2. Velocity
    Fig3. Magnetic Field