Solar Oblateness and Differentially Rotating Polytropes

1970 ◽  
pp. 352-355
Author(s):  
G. G. Fahlman ◽  
M. D. T. Naylor ◽  
S. P. S. Anand
Keyword(s):  
1975 ◽  
Vol 34 (5) ◽  
pp. 296-296
Author(s):  
H. A. Hill ◽  
P. D. Clayton ◽  
D. L. Patz ◽  
A. W. Healy ◽  
R. T. Stebbins ◽  
...  
Keyword(s):  

1967 ◽  
Vol 19 (10) ◽  
pp. 609-611 ◽  
Author(s):  
W. J. Cocke
Keyword(s):  

Science ◽  
2009 ◽  
Vol 324 (5931) ◽  
pp. 1143-1143 ◽  
Author(s):  
M. D. Fivian ◽  
H. S. Hudson ◽  
R. P. Lin ◽  
H. J. Zahid

Nature ◽  
1969 ◽  
Vol 221 (5181) ◽  
pp. 646-648 ◽  
Author(s):  
B. R. DURNEY ◽  
I. W. ROXBURGH

1973 ◽  
Vol 224 (1 Sixth Texas S) ◽  
pp. 316-327
Author(s):  
R. H. Dicke
Keyword(s):  

2011 ◽  
Vol 03 ◽  
pp. 464-474
Author(s):  
COSTANTINO SIGISMONDI

The modern methods of measurement of the solar diameter and oblateness are reviewed. Either ground-based or balloon-borne and satellite measurements are considered. The importance of solar astrometry for General Relativity is emphasized, particularly attention is given to the solar oblateness problem, as well as the studies of solar astrophysics to the whole world of physics from nucleosynthesis to neutrinos.


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