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

Relative heating of protons and electrons in the young solar wind due to turbulent dissipation mediated by Landau damping

Authors: Niranjana Shankarappa (University of Arizona), Kristopher Klein (University of Arizona) The heating of protons and electrons as the result of the dissipation of turbulenceView More

Towards Accurate Modeling of Pickup Ions in the  Solar Wind Interaction with the Local Interstellar Medium

Authors: Ratan Kumar Bera (Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville), Nikolai V Pogorelov (University of Alabama in Huntsville), FedericoView More

Properties of Coherent Magnetic Structures in Composition-Enhanced Solar Wind from the S-Web

Authors: B. J. Lynch (SSL/UCB), N. M. Viall (GSFC/NASA), A. K. Higginson (GSFC/NASA), L. Zhao (CLaSP/UM), S. T. Lepri (CLaSP/UM), X. Sun (IfA/UH) Connecting theView More

Polarimeter to UNify the Corona and Heliosphere (PUNCH)

Authors: Don Kolinski (High Altitude Observatory, National Center for Atmospheric Research), Craig DeForest (Southwest Research Institute), Sarah Gibson (High Altitude Observatory, National Center for AtmosphericView More

Observation and modeling of an geo-effective event observed on 2011 May 28 from the solar surface to 1AU

Authors: Nishu Karna(CfA), Tatiana Niembro(CfA) Coronal holes are the source of the fast solar wind, and thus play a crucial role in heliophysics as oneView More

Laboratory study of the stability of solar-relevant, arched, line-tied magnetic flux ropes

Authors: Andrew Alt (Princeton University), Hantao Ji (Princeton University), Jongsoo Yoo (Princeton Plasma Physics Laboratory), Sayak Bose (Princeton Plasma Physics Laboratory), Aaron Goodman (Princeton University),View More

Evidence for Parametric Decay Instability in the Lower Solar Atmosphere

Authors: Michael Hahn (Columbia University), Xiangrong Fu (New Mexico Consortium), Daniel Wolf Savin (Columbia University) We have found evidence for the parametric decay instability (PDI)View More

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