Inversion of the Internal Solar Rotation Rate

2002 ◽  
Vol 573 (2) ◽  
pp. 857-863 ◽  
Author(s):  
A. Eff‐Darwich ◽  
S. G. Korzennik ◽  
S. J. Jimenez‐Reyes

2021 ◽  
Author(s):  
Roger Ulrich ◽  
John Boyden ◽  
Tham Tran ◽  
Luca Bertello


1998 ◽  
Vol 499 (1) ◽  
pp. 504-512 ◽  
Author(s):  
Y. Li ◽  
P. R. Wilson


Author(s):  
Sylvain G. Korzennik ◽  
Alessandro Cacciani ◽  
Edward J. Rhodes ◽  
Roger K. Ulrich


2010 ◽  
Vol 331 (9-10) ◽  
pp. 890-895 ◽  
Author(s):  
A. Eff-Darwich ◽  
S.G. Korzennik ◽  
R.A. García


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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