Physics
Scientist
Alaska, University, Fairbanks, AK
A method for determining corotating interaction regions in the equatorial plane of the heliosphere from solar wind velocity data
A representation of the magnetic neutral line on the solar source surface in terms of the sun's axial dipole at the center and two equatorial dipoles in the photosphere
One-dimensional kinematics of particle stream flow with application to solar wind simulation
Quantitative forecasting of the 27-day recurrent magnetic activity
Solar activity and modulation of the cosmic ray intensity
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