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. DensityFig2. VelocityFig3. Magnetic Field