Solar coronal structure: A comparison of NSO/SP ground-based coronal emission line intensities and temperatures with Yohkoh SXT and WSO magnetic data

1996 ◽  
Vol 17 (4-5) ◽  
pp. 235-238 ◽  
Author(s):  
R.C Altrock ◽  
P Hick ◽  
B.V Jackson ◽  
J.T Hoeksema ◽  
X.P Zhao ◽  
...  
Keyword(s):  
Emission Line ◽  
Magnetic Data ◽  
Coronal Structure ◽  
Coronal Emission ◽  
Line Intensities ◽  
Coronal Emission Line ◽  
Solar Coronal

Coronal Emission-Line Intensities in the Extreme Ultraviolet

1966 ◽  
Vol 145 ◽  
pp. 373 ◽  
Author(s):  
W. E. Austin ◽  
J. D. Purcell ◽  
R. Tousey ◽  
K. G. Widing
Keyword(s):  
Emission Line ◽  
Extreme Ultraviolet ◽  
Coronal Emission ◽  
Line Intensities ◽  
Coronal Emission Line

A possible E-W asymmetry of the coronal emission line intensities and K-corona brightness

1994 ◽  
Vol 218 (1) ◽  
pp. 35-57 ◽  
Author(s):  
H. Mavromichalaki ◽  
V. Tritakis ◽  
B. Petropoulos ◽  
E. Marmatsouri ◽  
A. Vassilaki ◽  
...  
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Line Intensities ◽  
Coronal Emission Line

Coronal emission line polarization

Solar Physics ◽  
1972 ◽  
Vol 23 (1) ◽  
pp. 103-119 ◽  
Author(s):  
Lewis L. House
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Coronal Emission Line

How bright is the [Si X] 1431 nm coronal emission line?

Solar Physics ◽  
1994 ◽  
Vol 151 (1) ◽  
pp. 51-56 ◽  
Author(s):  
M. J. Penn ◽  
J. R. Kuhn
Keyword(s):  
Emission Line ◽  
Coronal Emission ◽  
Coronal Emission Line
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