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Gary Zank
Univ of Alabama, HuntsvilleMeeting roles in:
Energetic Proton Acceleration During the Interaction of an Interplanetary Shock and Current Sheet Structure
Solar Wind H+ and PUI H+ Heating Rates in the Outer Heliosphere
The Parallel and Perpendicular Diffusion Coefficient of Energetic Charged Particles in the Inner Heliosphere from the Turbulent Magnetic fields Measured by Parker Solar Probe.
On the energy spectrum of diffusive accelerated particles in the mediated shock
Survival of 2D Turbulence in the Local Interstellar Medium
The Impact of Physical Processes on the Radial Evolution of the Distant Pickup Ion Mediated Solar Wind
Modeling Coronal Loop Heating: Insights from Reduced Magnetohydrodynamic and Phenomenological Approaches
Heliophysics REU Program at The University of Alabama in Huntsville and NASA Marshall Space Flight Center: Celebrating 13 Years of Service to the US STEM Undergraduate Community
The Heliosheath with a Non-Maxwellian, Isotropic Pickup-Ion Distribution
Enter Note
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