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- W4243232103 abstract "The authors describe an investigation on the center-to-limb variation of the line asymmetry and shift along the polar and equatorial diameters of the Sun on two Fe I photospheric lines. The observations do not show any significant latitudinal dependence of the line asymmetry. Instead, the limb shift curves obtained along the polar diameter systematically differ from those obtained along the equator. This difference, if interpreted as due to a surface mass flow, implies a poleward meridional motion with a maximum of about 50m s-1 at 45° of latitude in both hemispheres. A detailed analysis of these and previous results suggests that the so called ”meridional motions”, found by spectroscopical means, mainly originate from latitudinal effects on the convective line shift, which might also be modulated by the activity cycle." @default.
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- W4243232103 date "1987-01-01" @default.
- W4243232103 modified "2023-09-27" @default.
- W4243232103 title "Sun" @default.
- W4243232103 doi "https://doi.org/10.1007/978-3-662-12382-9_10" @default.
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