126 citations · 666 across the 13 of their papers we have counts for
13 papers
For SIRs, CIRs, and Beyond: Polarization Ratio to Feature Location
Curt A. de Koning, Dusan Odstrcil, Sarah Gibson +3
The Polarimeter to UNify the Corona and Heliosphere (PUNCH) mission will remotely observe solar wind transients with high signal-to-noise ratio, high-cadence, high-resolution polar…
A Chromatic Treatment of Linear Polarization in the Solar Corona at the 2023 Total Solar Eclipse
Ritesh Patel, Daniel B. Seaton, Amir Caspi +17
The broadband solar K-corona is linearly polarized due to Thomson scattering. Various strategies have been used to represent coronal polarization. Here, we present a new way to vis…
Shear-Driven Transition to Isotropically Turbulent Solar Wind Outside the Alfven Critical Zone
D. Ruffolo, W. H. Matthaeus, R. Chhiber +11
Motivated by prior remote observations of a transition from striated solar coronal structures to more isotropic ``flocculated'' fluctuations, we propose that the dynamics of the in…
Noise-gating to clean astrophysical image data
C. E. DeForest
I present a family of algorithms to reduce noise in astrophysical im- ages and image sequences, preserving more information from the original data than is retained by conventional…
Spatial Nonlocality of the Small-Scale Solar Dynamo
Derek A. Lamb, Timothy A. Howard, Craig E. DeForest
We explore the nature of the small-scale solar dynamo by tracking magnetic features. We investigate two previously-explored categories of the small-scale solar dynamo: shallow and…
Sparkling EUV bright dots observed with Hi-C
S. Regnier, C. E. Alexander, R. W. Walsh +12
Observing the Sun at high time and spatial scales is a step towards understanding the finest and fundamental scales of heating events in the solar corona. The Hi-C instrument has p…