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Image instabilities and polarization cross-talk

polarization cross-talk

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

Graph of polarimetric errors

A unifying polarization formalism for electric- and magnetic-multipole interactions

Hanle diagrams

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

Diagnostic Potential of a Coronal Emission Line

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

Alfred De Wijn and Roberto Cassini installing ViSP

Effects of spectral resolution on simple magnetic field diagnostics of the Mg II h & k lines

3 Scatter density plots of the retrieved value of Blos

Optimal spectral lines for measuring chromospheric magnetic fields

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

P Judge and R Casini Advise Early Career Researchers

Phil Judge and Roberto Cassini

On single-point inversions of magnetic dipole lines in the corona

scattering geometry of point P is shown in the observer's frame with projections of the magnetic field components in this frame
Subscribe to Roberto Casini

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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.