An extended and fragmented Alfvén zone in the Young Solar Wind

Authors: Rohit Chhiber (University of Delaware & NASA GSFC), William Matthaeus (University of Delaware), Arcadi Usmanov (University of Delaware & NASA GSFC), Riddhi Bandyopadhyay (PrincetonView More

What is a Better Way for Data-based Solar Magnetohydrodynamic Simulations?

Authors: Satoshi Inoue (Center for Solar-Terrestrial Research, New Jersey Institute of Technology), Keiji Hayashi (George Mason University), Takahiro Miyoshi (Graduate School of Science, Hiroshima UniversityView More

Ion cyclotron waves in the solar wind and their indications of source ion distributions

Authors: H. Y. Wei (Dept. of Earth, Planetary and Space Sciences, University of California, Los Angeles, CA, USA), L. K. Jian (NASA Goddard Space FlightView More

Investigating the Asymmetry of the Magnetic Field Profile of “Simple” Magnetic Ejecta

Authors: Wenyuan Yu (University of New Hampshire), Nada A. Al-Haddad (University of New Hampshire), Charles J. Farrugia (University of New Hampshire), Noé Lugaz (University ofView More

Human Exploration Operations and the Need for Validating Space Weather Models

Authors: Philip Quinn (NASA/JSC/SRAG (Leidos)) In human exploration operations, space weather forecasting models are used to help predict the severity of solar particle events. ButView More

Investigating the radial evolution of solar wind structures with PSP’s 11th Encounter

Authors: S.D. Bale, T. S. Horbury, L.Matteini, T. Woolley, J. Stawarz, L.D. Woodham Parker Solar Probe’s (PSP’s) 11th encounter in February 2022 has provided aView More

Phase Space Energization Analysis of the Corrugation Instability using the Field-Particle Correlation Technique

Authors: Collin Brown (University of Iowa), James Juno (Princeton Plasma Physics Laboratory), Greg Howes (University of Iowa), Colby Haggerty (University of Hawaii), Sage Constantinou (UniversityView More

The Mesoscale Structure of Three Unremarkable Coronal Mass Ejections observed near Earth

Authors: Rachael Filwett (University of Iowa), Joe Fennell (Aerospace Corporation), Bern Blake (Aerospace Corporation), Allison Jaynes (University of Iowa), Drew Turner (APL), Robert Allen (APL)View More

Eruptive vs. confined solar flares: statistical comparison of their solar source properties

Authors: Maria D. Kazachenko (CU Boulder / NSO) What is the difference between confined and eruptive flares in terms of their physical properties at theView More

Predicting Solar Wind Footpoints as Probability Distributions using WSA/ADAPT

Authors: Daniel da Silva (NASA/GSFC, UMBC), Nick Arge (NASA/GSFC), Shaela Jones (NASA/GSFC, Catholic University), Samantha Wallace (NASA/GSFC) The origin point on the sun corresponding toView More

Classification of Solar Wind Instabilities in the Inner Heliosphere

Authors: Mihailo M. Martinovic (University of Arizona), Kristopher G. Klein (University of Arizona), Tereza Durovcova (Charles University, Prague), Benjamin L. Alterman (Southwest Research Institute) InstabilitiesView More

Emulating Coronal Field Models with Physics-Informed Neural Nets

Authors: Nathaniel H. Mathews (NASA GSFC), Barbara J. Thompson (NASA GSFC) Predicting the current or future state of the coronal magnetic field requires high-resolution modelsView More

HelioSwarm: Characterizing the Multi-Scale Nature of Space Plasma Turbulence

Authors: K.G. Klein, H. Spence, & the HelioSwarm Science and Engineering Teams Turbulence is multiscale disorder. It arises in a variety of astrophysical and heliosphericView More

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