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Polarimetry and PSFs: Behind the Scenes with PUNCH Data Analysis

ECCCO: The EUV CME and Coronal Connectivity Observatory

Probing Chromospheric Temperatures and Dynamics with ALMA

Ultraviolet Spectropolarimetry: A New Diagnostic Window In Solar Physics

Optimally depth-resolved photospheric inversions using the iterative OLA method and tool for optimal spectral line selection

Towards Understanding the Initiation and Acceleration of Coronal Jets

Long-Lasting Solar Coherent Radio Bursts and Implications for Solar–Stellar Connection

Inferring Fundamental Properties of the Flare Current Sheet Using Flare Ribbons: Oscillations in the Reconnection Flux Rates

Nov 9, 2pm MT

The Topology of Magnetic Fields in Solar Active Regions

2pm MT

Collisional Shearing: A Possible Mechanism Producing Recurrent Explosive (Flare and CME) Activity in Solar Active Regions

Wed Oct 12, 2pm MT

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This material is based upon work supported by the NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the U.S. National Science Foundation.