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SynCOM: An Empirical Model for High-Resolution Simulations of Transient Solar Wind Flows

COR2 and a SynCOM simulated image

A Study on the Nested Rings CME Structure Observed by the WISPR Imager Onboard Parker Solar Probe

CME analysis

Observing the evolution of the Sun’s global coronal magnetic field

Gibson Coronal Activity

EUV polarimetric diagnostics of the solar corona: the Hanle effect of Ne viii 770 A

Diagnostic Potential of a Coronal Emission Line

Magnetohydrodynamic turbulence simulations as a testing ground for PUNCH

Magnetohydrodynamic Simulations of Turbulence

WHPI repository of 2024 Total Solar Eclipse activities

WHPI campaign April 8, 2024 total solar eclipse

Comprehensive analysis of a filament-embedding solar active region at different stages of evolution

NVST and CHASE observations, Feb 14

Mapping the Sun’s Alfvén Surface with PUNCH

Inflows towards Bipolar Magnetic Active Regions and Their Nonlinear Impact on a Three-Dimensional Babcock-Leighton Solar Dynamo Model

Cycling magnetic behavior

International UCoMP Users Workshop

UCoMP Users Workshop

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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.