2 citations · 2 across the 5 of their papers we have counts for
5 papers
PRICM3: A novel Polarization Ratio framework for three-dimensional CME reconstruction
Yara De Leo, Manuela Temmer, Fernando M. López +15
Coronal mass ejections (CMEs) are inherently three-dimensional (3D), but traditional white-light coronagraphs provide only two-dimensional (2D) projections. While the Polarization…
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…
Joint Diagnostics of Circumsolar Sky Brightness Using Coronagraphic Measurements and Aerosol Optical Inversions at Mauna Loa
Thomas A. Schad, Paul Bryans, Andre Fehlmann +5
Atmospheric aerosols strongly influence daytime sky quality for solar coronal imaging, yet few studies directly link aerosol properties and sky-brightness measurements within ~2° o…
SynCOM: A tool for simulating coronal outflows
Valmir Moraes Filho, Vadim Uritsky, Barbara Thompson +2
SynCOM is a package of procedures written in IDL (Interactive Data Language) that simulates transient solar wind flows. Each function within SynCOM handles specific tasks, such as…
SynCOM: An Empirical Model for High-Resolution Simulations of Transient Solar Wind Flows
Valmir P. Moraes Filho, Vadim M. Uritsky, Barbara J. Thompson +2
The Synthetic Corona Outflow Model (SynCOM), an empirical model, simulates the solar corona's dynamics to match high-resolution observations, providing a useful resource for testin…