| Automated detection and tracking of CMEs using HI instruments |
Maike Bauer, Austrian Space Weather Office, GeoSphere Austria, Graz, Austria |
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| Synergies of ground-based solar observations with PUNCH NFI and other space-based coronagraphs |
Joan Burkepile, National Center for Atmospheric Research / HAO |
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| Statistical Relationships Between Solar Wind Parameters: Implications for Space Weather Forecasts |
Heather Elliott, Southwest Research Institute |
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| An Association between the fast CME shocks and radio signatures |
Syed Ibrahim M, Postdoctoral Fellow, Indian Institute of Astrophysics |
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| Low frequency 1/f noise in the solar atmosphere |
Bill Matthaeus, University of Delaware |
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| SynCOM: An Empirical Model for High-Resolution Simulations of Transient Solar Wind Flows |
Valmir Moraes Filho, Catholic University of America at NASA/GSFC |
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| Magnetohydrodynamic turbulence simulations as a testing ground for PUNCH |
Francesco Pecora, University of Delaware |
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| Periodic Density Structures from Ulysses |
Brent Randol, NASA/GSFC |
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| Exploring Shocks in the Heliosphere for SEP producing CMEs with SoloHI Observations |
Shaheda Begum Shaik, George Mason University/Naval Research Laboratory |
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| PUNCH as an Open Science Mission |
Barbara Thompson, NASA GSFC |
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| Data-Driven Reconstruction of the Large-Scale Open-Flux Coronal Magnetic Field Using QRaFT Technique |
Vadim Uritsky, CUA at NASA/GSFC |
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| Reconstructing the 3D Solar Wind Speed in the Middle Corona with Metis. |
Alberto Vasquez, Instituto de Astronomía y Física del Espacio (IAFE, UBA-CONICET) Buenos Aires - Argentina |
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| Periodic Solar Wind Density Structures |
Nicholeen Viall, NASA Goddard Space Flight Center |
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