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Solar Wind Mass‐Loss Rate and Its Dependence on Open Solar Magnetic Flux During Solar Cycles 23–25

Zavkiddin MirtoshevInstitute of Nuclear Technologies Samarkand State University Samarkand UzbekistanAkmal SafarovInstitute of Nuclear Technologies Samarkand State University Samarkand UzbekistanShakhboz KhasanovInstitute of Nuclear Technologies Samarkand State University Samarkand Uzbekistan

Astronomische Nachrichtenjournal2026en

ABI

Annotatsiya

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.

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Mavzular

Solar and Space Plasma Dynamics Ionosphere and magnetosphere dynamics Geomagnetism and Paleomagnetism Studies

Identifikatorlar

DOI: 10.1002/asna.70099

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