activity
20192025
most citedThe Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

112 citations · 394 across the 21 of their papers we have counts for

collaborators
Showing 2023Show all

6 papers · 1 filter

astro-ph.SR2023

Ensemble Forecasts of Solar Wind Connectivity to 1 Rs using ADAPT-WSA

D. E. da Silva, S. Wallace, C. N. Arge +1

The solar wind which arrives at any location in the solar system is, in principle, relatable to the outflow of solar plasma from a single source location. This source location, its…

astro-ph.SR2023★ 8 cited

Quantifying the Consistency and Characterizing the Confidence of Coronal Holes Detected by Active Contours without Edges (ACWE)

Jeremy A. Grajeda, Laura E. Boucheron, Michael S. Kirk +2

Coronal Holes (CHs) are regions of open magnetic field lines, resulting in high speed solar wind. Accurate detection of CHs is vital for space weather prediction. This paper presen…

astro-ph.SR2023

Proposed Resolution to the Solar Open Magnetic Flux Problem

C. Nick Arge, Andrew Leisner, Samantha Wallace +1

The solar magnetic fields emerging from the photosphere into the chromosphere and corona are comprised of a combination of "closed" and "open" fields. The closed magnetic field lin…

astro-ph.SR2023★ 44 cited

Prediction and Verification of Parker Solar Probe Solar Wind Sources at 13.3 R

Samuel T. Badman, Pete Riley, Shaela I. Jones +11

Drawing connections between heliospheric spacecraft and solar wind sources is a vital step in understanding the evolution of the solar corona into the solar wind and contextualizin…

astro-ph.SR2023★ 17 cited

Implications of Different Solar Photospheric Flux-Transport Models for Global Coronal and Heliospheric Modeling

Graham Barnes, Marc L. DeRosa, Shaela I. Jones +3

The concept of surface-flux transport (SFT) is commonly used in evolving models of the large-scale solar surface magnetic field. These photospheric models are used to determine the…

physics.space-ph2023★ 15 cited

Improving the Arrival Time Estimates of Coronal Mass Ejections by Using Magnetohydrodynamic Ensemble Modeling, Heliospheric Imager data, and Machine Learning

Talwinder Singh, Bernard Benson, Syed A. Z. Raza +4

The arrival time prediction of Coronal mass ejections (CMEs) is an area of active research. Many methods with varying levels of complexity have been developed to predict CME arriva…