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Solar Surface Magnetic Field Simulation Enabled Prediction of the Large-Scale Coronal Structure of the 21 August 2017 Great American Eclipse: An Assessment of Model Predictions and Observations
Dibyendu Nandy, Prantika Bhowmik, Anthony R. Yeates +3
On 21 August 2017 a total solar eclipse swept across the contiguous United States providing excellent opportunities for diagnostics of the Sun's corona. The Sun's coronal structure…
Impact of Non-potential Coronal Boundary Conditions on Solar Wind Prediction
Marion Weinzierl, Francois-X. Bocquet, Anthony R. Yeates
Predictions of the solar wind at Earth are a central aspect of space weather prediction. The outcome of such a prediction, however, is highly sensitive to the method used for compu…
The Open Flux Problem
J. A. Linker, R. M. Caplan, C. Downs +9
The heliospheric magnetic field is of pivotal importance in solar and space physics. The field is rooted in the Sun's photosphere, where it has been observed for many years. Global…
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…
Sparse reconstruction of electric fields from radial magnetic data
A. R. Yeates
Accurate estimates of the horizontal electric field on the Sun's visible surface are important not only for estimating the Poynting flux of magnetic energy into the corona but also…