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• W1818653604 abstract "We have studied the relationship between the solar-wind speed $[V]$ and the coronal magnetic-field properties (a flux-expansion factor [ $f$ ] and photospheric magnetic-field strength [ $B_{mathrm{S}}$ ]) at all latitudes using data of interplanetary scintillation and solar magnetic field obtained for 24 years from 1986 to 2009. Using a cross-correlation analyses, we verified that $V$ is inversely proportional to $f$ and found that $V$ tends to increase with $B_{mathrm{S}}$ if $f$ is the same. As a consequence, we find that $V$ has an extremely good linear correlation with $B_{mathrm{S}}/f$ . However, this linear relation of $V$ and $B_{mathrm{S}}/f$ cannot be used for predicting the solar-wind velocity without information on the solar-wind mass flux. We discuss why the inverse relation between $V$ and $f$ has been successfully used for solar-wind velocity prediction, even though it does not explicitly include the mass flux and magnetic-field strength, which are important physical parameters for solar-wind acceleration." @default.
• W1818653604 created "2016-06-24" @default.
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• W1818653604 date "2015-07-30" @default.
• W1818653604 modified "2023-10-16" @default.
• W1818653604 title "Relationship Between Solar-Wind Speed and Coronal Magnetic-Field Properties" @default.
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• W1818653604 doi "https://doi.org/10.1007/s11207-015-0742-8" @default.
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