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Chasing the IR Corona through Solar Eclipse Experiments

2024 Total Solar Eclipse Composite

WHPI repository of 2024 Total Solar Eclipse activities

WHPI campaign April 8, 2024 total solar eclipse

International UCoMP Users Workshop

UCoMP Users Workshop

Optimal spectral lines for measuring chromospheric magnetic fields

The solar spectrum seen at low resolution, below the atmospheric cutoff at 3100 Angstrom

Paul Bryans interviewed by Sun Superheroes

Solar Eclipse Team, Chile, 2019

AAS Nova Features a Recent Publication by Philip Judge

Images to highlight the corrugated surfaces at which the centers of UV lines are formed (close to τ = 1) in MURaM calculations of the upper solar chromosphere

A new facility for airborne solar astronomy: NASA’s WB-57 at the 2017 total solar eclipse

Fully processed image of the corona generated by stacking many co-aligned, calibrated images and applying a radial filter and multi-scale unsharp mask to bring out details at higher altitudes

Detecting the Chromospheric Footpoints of the Solar Wind

SDO and IRIS full-disk observations from 2016 Feb 22
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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.