The Impact of Time-Dependent WSA Boundary Conditions on Magnetic Connectivity and Mesoscale Solar Wind Structure
Time-dependent (TD) heliospheric simulations driven by evolving Wang-Sheeley-Arge (WSA) model boundary conditions are increasingly relevant for improving heliospheric solar wind modeling. In this study, we quantify the differences between TD and stead
Authors
- Chaitanya Prasad Sishtla (ORCID: https://orcid.org/0000-0003-4236-768X)
- Davide Manzini
- Luke Barnard (ORCID: https://orcid.org/0000-0001-9876-4612)
- Pauline A. Simon (ORCID: https://orcid.org/0000-0003-2091-2093)
- Christopher H. K. Chen (ORCID: https://orcid.org/0000-0003-4529-3620)
- Jens Pomoell (ORCID: https://orcid.org/0000-0003-1175-7124)
Institutions
- University of Helsinki (FI)
- Queen Mary University of London (GB)
- University of Reading (GB)
Publication Details
- Published
- 2025-09-29
- DOI
- https://doi.org/10.22541/essoar.175917081.12209420/v1
- Primary Topic
- Solar and Space Plasma Dynamics
- Type
- article
- Field-Weighted Citation Impact
- 0.00
Funders
- Queen Mary University of London
- UK Research and Innovation
- Science and Technology Facilities Council