scholarly journals Time Dependence of the Solar Rotation Rate

2021 ◽  
Author(s):  
Roger Ulrich ◽  
John Boyden ◽  
Tham Tran ◽  
Luca Bertello
2010 ◽  
Vol 720 (1) ◽  
pp. 494-502 ◽  
Author(s):  
H. M. Antia ◽  
Sarbani Basu

Solar Physics ◽  
1985 ◽  
Vol 97 (1) ◽  
pp. 203-212 ◽  
Author(s):  
Jagdev Singh ◽  
T. P. Prabhu

2008 ◽  
Vol 681 (1) ◽  
pp. 680-692 ◽  
Author(s):  
H. M. Antia ◽  
Sarbani Basu ◽  
S. M. Chitre

1988 ◽  
Vol 123 ◽  
pp. 49-52
Author(s):  
Frank Hill ◽  
David M. Rust ◽  
Thierry Appourchaux

Full disk observations of the 5-min solar oscillations have been obtained with a lithium niobate Fabry-Perot filter. The equatorial solar rotation rate as a function of depth has been inferred from the sectoral modes of oscillation using the Backus-Gilbert optimal averaging inversion method. The results show a rotation rate that slowly decreases over the depths of 15 to 56 Mm below the photosphere. The results are in agreement with the previous Duvall-Harvey observations.


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