Phase Relations Between Variations in Solar Surface Velocity and Magnetic Fields
Lead Investigator:
R.K. Ulrich
Team Members:
A.A. Norton
Technical Summary:
We propose to determine the phase relations between variations
in velocities and magnetic fields in the solar photosphere.
The observed phase relations will provide information about
the generation and propogation of Alfven waves in the solar
atmosphere and the consequent energy flux. The study will
utilize SOI-MDI high resolution campaign data and possible
some high-rate continuing observing sequences which return
near simultaneous images of surface velocity and magnetic
fields.
Complete text of proposal.