activity
20152025
most citedMeasurements of EUV Coronal Holes and Open Magnetic Flux

50 citations · 84 across the 5 of their papers we have counts for

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Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2025

Direct calculation of steady-state hydrodynamic solar wind solutions with newtonian viscosity

Roger B. Scott, Stephen J. Bradshaw, Mark G. Linton +2

Steady-state solutions to the Navier-Stokes equations are known to admit solutions that are singular at the sonic point. Consequently, inviscid solar wind models require special tr…

astro-ph.SR20259 cited

Polarimeter to Unify the Corona and Heliosphere (PUNCH)

Craig E. DeForest, Sarah E. Gibson, Ronnie Killough +74

The Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission is a NASA Small Explorer to determine the cross-scale processes that unify the solar corona and heliosphere. PUN…

astro-ph.SR2024

Field Line Universal relaXer (FLUX): A Fluxon Approach to Coronal Magnetic Field Modeling

Chris Lowder, Chris Gilly, Craig DeForest

We describe a novel method for modeling the global, steady solar wind using photospheric magnetic fields as a driving boundary condition. Prior wind models in this class include bo…

astro-ph.SR2021

The Observational Uncertainty of Coronal Hole Boundaries in Automated Detection Schemes

Martin A. Reiss, Karin Muglach, Christian Möstl +16

Coronal holes are the observational manifestation of the solar magnetic field open to the heliosphere and are of pivotal importance for our understanding of the origin and accelera…

astro-ph.SR2018

Global Non-Potential Magnetic Models of the Solar Corona During the March 2015 Eclipse

A. R. Yeates, T. Amari, I. Contopoulos +17

Seven different models are applied to the same problem of simulating the Sun's coronal magnetic field during the solar eclipse on 2015 March 20. All of the models are non-potential…

astro-ph.SR201725 cited

Magnetic Flux Rope Identification and Characterization from Observationally-Driven Solar Coronal Models

Chris Lowder, Anthony Yeates

Formed through magnetic field shearing and reconnection in the solar corona, magnetic flux ropes are structures of twisted magnetic field, threaded along an axis. Their evolution a…