Alonso Guzmán, J. G. https://orcid.org/0000-0001-9581-3167
Florinski, V. https://orcid.org/0000-0001-5485-2872
Zhao, L.-L. https://orcid.org/0000-0002-4299-0490
Cummings, A. C. https://orcid.org/0000-0002-3840-7696
Heikkila, B. C.
Hill, M. E. https://orcid.org/0000-0002-5674-4936
Nikoukar, R. https://orcid.org/0000-0002-8608-2822
Opher, M. https://orcid.org/0000-0002-8767-8273
Funding for this research was provided by:
NASA ∣ SMD ∣ Heliophysics Division (80NSSC20K0603)
NASA ∣ SMD ∣ Heliophysics Division (80NSSC24K0568)
NSF ∣ CISE ∣ Office of Advanced Cyberinfrastructure (2514037)
NSF ∣ GEO ∣ Division of Atmospheric and Geospace Sciences (2442628)
NASA ∣ SMD ∣ Heliophysics Division (80NSSC20K1783)
NASA ∣ SMD ∣ Heliophysics Division (80NSSC23K0415)
NASA ∣ SMD ∣ Heliophysics Division (80NM0018F0577)
NASA ∣ SMD ∣ Heliophysics Division (NNN06AA01C)
Article Title: Toward Explaining Galactic Cosmic-Ray Modulation in a Dynamic Heliosheath: Transient Structures Seem Dominant and Magnetic Drifts Appear Reduced
Journal Title: The Astrophysical Journal
Article Type: paper
Copyright Information: © 2026. The Author(s). Published by the American Astronomical Society.
Publication dates
Date Received: 2026-02-20
Date Accepted: 2026-04-04
Online publication date: 2026-04-28