Solar Wind Mass‐Loss Rate and Its Dependence on Open Solar Magnetic Flux During Solar Cycles 23–25
ABSTRACT We investigate the solar wind mass‐loss rate and its relationship with open solar magnetic flux (OSF) over Solar Cycles 23–25 using OMNI, SIDC, and SOHO/LASCO data. The solar wind mass‐loss rate correlates more strongly with OSF than with sunspot number, establishing OSF as a superior predictor of heliospheric mass‐loss.
Authors
- Shakhboz Khasanov (ORCID: https://orcid.org/0000-0001-6787-9492)
- Zavkiddin Mirtoshev (ORCID: https://orcid.org/0000-0002-1984-2254)
- Akmal Safarov
Institutions
- Samarkand State University named after Sharof Rashidov (UZ)
Publication Details
- Journal
- Astronomische Nachrichten
- Published
- 2026-04-17
- DOI
- https://doi.org/10.1002/asna.70099
- Primary Topic
- Solar and Space Plasma Dynamics
- Type
- article
- Field-Weighted Citation Impact
- 0.00