The Corona of the Sun

Author(s):  
Ephraim Miller
Keyword(s):  
The Sun ◽  

2015 ◽  
Vol 11 (6) ◽  
pp. 492-495 ◽  
Author(s):  
F. Chen ◽  
H. Peter ◽  
S. Bingert ◽  
M. C. M. Cheung
Keyword(s):  
The Sun ◽  


Author(s):  
Takao Saito ◽  
S.-I. Akasofu ◽  
Y. Kozuka ◽  
S. Minami ◽  
S. Tuneta


2016 ◽  
Vol 50 (2) ◽  
pp. 143-160 ◽  
Author(s):  
L. I. Shestakova ◽  
B. I. Demchenko


2004 ◽  
Vol 45 (4) ◽  
pp. 4.26-4.27 ◽  
Author(s):  
V M Nakariakov ◽  
E Verwichte
Keyword(s):  
The Sun ◽  


Science ◽  
1937 ◽  
Vol 86 (2225) ◽  
pp. 8-8
Keyword(s):  
The Sun ◽  


1886 ◽  
Vol 39 (239-241) ◽  
pp. 108-135 ◽  

The sun is the only star the corona of which we have been able to observe, for all other stars are too distant to give true images in the telescope. If the sun were removed to a distance equal to that of the nearest star, its disk would subtend less than the one-hundredth of a second of arc. We have also to consider the small relative brightness of the corona, the light from which has been estimated at different times to be from 1/100000 to about the 1/400000 part of the sun’s light. It is, indeed, possible that stars which have a higher temperature than our sun, are surrounded by coronæ of greater extent and brightness.



Solar Physics ◽  
2006 ◽  
Vol 237 (1) ◽  
pp. 201-210 ◽  
Author(s):  
V. I. Makarov ◽  
A. G. Tlatov ◽  
D. K. Callebaut
Keyword(s):  
The Sun ◽  


2006 ◽  
Author(s):  
Giovanni Peres
Keyword(s):  
The Sun ◽  




2009 ◽  
Author(s):  
M. A. Livshits ◽  
M. M. Katsova ◽  
I. M. Livshits ◽  
J. Sykora ◽  
Eric Stempels


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