The Vector Tomographic Inversion for the Solar Coronal Magnetic Field with DKIST and UCoMP instruments.

Authors: Maxim Kramar (University of Hawaii at Manoa), Haosheng Lin (University of Hawaii at Manoa) The coronal magnetic field is important driving force for transientView More

Nowcasting and forecasting SEP events with the iPATH model

Authors: Junxiang Hu (UAH), Gang Li (UAH) This work showcases the nowcasting and forecasting capabilities of the operational version of the iPATH (improved Particle AccelerationView More

FETCH concept: Investigating Quiescent and Transient Magnetic Structures in the Inner Heliosphere using Faraday Rotation of Spacecraft Radio Signals

Authors: Megan Kenny (University of Colorado, Boulder) Liz Jensen (Planetary Science Institute) Shing F. Fung, Lynn Wilson III, Lan Jian, Nat Gopalswamy, Teresa Nieves-Chinchilla (HeliophysicsView More

Guide field dependence of energy spectrum and energy transfer in reconnection

Authors: Michael Shay(University of Delaware), Tulasi N. Parashar (Victoria University of Wellington), William H. Matthaeus (University of Delaware) Classic picture of magnetic reconnection has shownView More

SOFIE (Solar-wind with Field-lines and Energetic-particles): A data-driven and self-consistent SEP modeling and forecasting tool

Authors: Lulu Zhao (University of Michigan), Igor Sokolov (University of Michigan), Tamas Gombosi (University of Michigan), Zhenguang Huang (University of Michigan), Gabor Toth (University ofView More

Acceleration of Solar Energetic Particles (SEPs) through a CME-driven Shock and Streamer Interaction

Authors: Matthew West (Southwest Research Institute), Federica Frassati (National Institute of Astrophysics – Astrophysical Observatory of Turin), Monica Laurenza (Istituto di Astrofisica e Planetologia Spaziali),View More

Modeling the Solar Wind During Different Phases of the Last Solar Cycle

Authors: Gabor Toth (University of Michigan), Nishtha Sachdeva (University of Michigan), Lulu Zhao (University of Michigan), Bart van der Holst (University of Michigan), Igor SokolovView More

Advantages of Characterising the Suprathermal Electrons Pitch-angle Distribution

Authors: Fernando Carcaboso (NASA Goddard Space Flight Center, The Catholic University of America), Raúl Gómez-Herrero (Space Research Group, University of Alcalá), Francisco Espinosa Lara (SpaceView More

Quantifying the Impacts of Interplanetary Propagation and Transient Events on Solar Energetic Particle Intensity-Time Profiles

Authors: Alicia K. Petersen (Air Force Research Lab, NRC), Stephen M. White (Air Force Research Lab, Kirtland AFB), Stephen W. Kahler (Air Force Research Lab,View More

The Variation of the Pitch-angle Distribution of 500 MeV solar protons at 1 au in a Weak Pitch-angle Scattering and in the Large-scale Turbulent Interplanetary Magnetic Field

Authors: Ashraf Moradi (University of Arizona), Joe Giacalone (University of Arizona) Solar protons with rigidities higher than 1 GV (432 MeV) penetrate Earth’s atmosphere, generateView More

The First Absolute Brightness Measurements and MHD Model Predictions of Fe X, XI, and XIV out to 3.4 Rs

Authors: Benjamin Boe (NSF Postdoctoral Fellow. Institute for Astronomy, University of Hawaii), Shadia Habbal (Institute for Astronomy, University of Hawaii), Cooper Downs (Predictive Science Inc.),View More

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