Phil Judge | High Altitude Observatory

On the intermittency of hot plasma loops in the solar corona

SDO and DKIS data

Erratum: Analysis of Seeing-Induced Polarization Cross-Talk and Modulation Scheme Performance

Graph of polarimetric errors

Magnetic fields beneath active region coronal loops

Instead heating arises within primarily unipolar fields above the chromosphere.

New Book! The Problem of Coronal Heating: A Rosetta Stone for Electrodynamic Coupling in Cosmic Plasmas

Cover of Phil Judge's book, The Problem of Coronal Heating

New Book: The Problem of Coronal Heating

The Problem of Coronal Heating

Magnetic fields and plasma heating in the Sun’s atmosphere

Comparison between DKIST and IRIS/SDO measurements

Steadiness of coronal heating

Solar Orbiter EUI revelations

First Observation of Chromospheric Waves in a Sunspot by DKIST/ViSP

Chromospheric Waves in a Sunspot by DKISTViSP

First Observation of Chromospheric Waves in a Sunspot by DKIST/ViSP

Predrag Sekulic (former DKIST optical engineer lead, left) and Robert Casini (right) installing ViSP

Derivation of Instrument Requirements for Polarimetry using Mg, Fe, and Mn lines between 250 and 290 nm

IRIS map

Subscribe to Phil Judge