On the determination of meridional flow on the Sun by the method of tracers
S. V. Olemskoy, L. L. Kitchatinov
Abstract
S. V. Olemskoy, L. L. Kitchatinov
Abstract
The standard methods for determining the meridional flow on the Sun from the motions of tracers are shown to give an error related to the latitudinal nonuniformity of the tracer distribution. We suggest a simple method for eliminating this error. Using this method to determine the meridional circulation from the motions of sunspots brings the result into agreement with helioseismological data on the meridional flow. The discussed effects can be important for observations of meridional flows on stars.
OpenAlex reports 19 citations for this work. Citation counts describe recorded attention and do not establish research quality.
A contribution statement is not available in the OpenAlex record.
Method details are not available in the OpenAlex metadata.
Findings are not separately available in the OpenAlex metadata.
Limitations are not available in the OpenAlex metadata.
Application details are not available in the OpenAlex metadata.
The standard methods for determining the meridional flow on the Sun from the motions of tracers are shown to give an error related to the latitudinal nonuniformity of the tracer distribution. We suggest a simple method for eliminating this error. Using this method to determine the meridional circulation from the motions of sunspots brings the result into agreement with helioseismological data on the meridional flow. The discussed effects can be important for observations of meridional flows on stars.
Key concepts: Zonal and meridional, Meridional flow, Physics, Sunspot, Flow (mathematics), Circulation (fluid dynamics), TRACER, Atmospheric sciences