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