UCoMP mounted on MLSO spar
Mar 4, 2022

UCoMP Instrument Nearing Science Mission Phase

Snapshot from a two-dimensional test simulation setup with a 8x8Mm domain reaching from the upper convection zone into the transition region
Mar 3, 2022

Efficient numerical treatment of ambipolar and Hall drift as hyperbolic system

Maps of the magnetic field strength at depth of z = −7.5 Mm beneath the solar photosphere at different times (indicated in red in each panel)
Mar 3, 2022

On the (In)stability of Sunspots

Solar Eclipse Team, Chile, 2019
Dec 20, 2021

Paul Bryans interviewed by Sun Superheroes

COSMO LC building
Nov 22, 2021

NSF Approves Funding For COSMO

Sunspot simulations
Nov 18, 2021

Opposite Polarity Magnetic Fields and Convective Downflows in a Simulated Sunspot Penumbra

Radial profiles of continuum intensity (b), magnetic field inclination (c), total magnetic field strength (d), vertical magnetic field strength (e), and horizontal magnetic field strength (f)
Nov 18, 2021

A distinct magnetic property of the inner penumbral boundary III. Analysis of simulated sunspots

Plots of magnetic field and TSI with time
Nov 17, 2021

On the contribution of quiet Sun magnetism to solar irradiance variations: Constraints on quiet Sun variability and grand minimum scenarios

White light images (upper panels A and B) from HAO's KCOR instrument are shown with Fe XIII emission line polarization data (HAO's CoMP instrument) acquired one day after the initial flare was released
Nov 16, 2021

Dynamics of Late-Stage Reconnection in the 2017 September 10 Solar Flare

Analysis results for the observation on November 3, 2016 (dataset D2)
Nov 16, 2021

Mapping the magnetic field in the solar corona through magnetoseismology

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