The solar spectrum seen at low resolution, below the atmospheric cutoff at 3100 Angstrom
Jul 11, 2022

Optimal spectral lines for measuring chromospheric magnetic fields

Solar Eclipse Team, Chile, 2019
Dec 20, 2021

Paul Bryans interviewed by Sun Superheroes

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
Nov 18, 2021

AAS Nova Features a Recent Publication by Philip Judge

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
Nov 18, 2021

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

SDO and IRIS full-disk observations from 2016 Feb 22
Nov 16, 2021

Detecting the Chromospheric Footpoints of the Solar Wind

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