On green-to-red line intensity ratio in the solar corona

Solar Physics ◽  
1976 ◽  
Vol 46 (1) ◽  
pp. 183-184 ◽  
Author(s):  
S. Chandra ◽  
U. Narain
Keyword(s):  
Solar Corona ◽  
Line Intensity ◽  
Intensity Ratio ◽  
Line Intensity Ratio ◽  
Red Line

On the Green-To-Red Line Intensity Ratio in the Solar Corona

1978 ◽  
Vol 33 (7) ◽  
pp. 786-788
Author(s):  
H. P. Mital ◽  
U. Narain
Keyword(s):  
Solar Corona ◽  
Line Intensity ◽  
Intensity Ratio ◽  
Radiative Recombination ◽  
Dielectronic Recombination ◽  
Coronal Temperature ◽  
Line Intensity Ratio ◽  
Intensity Ratios ◽  
Red Line

Green-to-red line intensity ratios have been investigated by including various processes, like radiative recombination via bound levels, autoionization, dielectronic recombination, etc. An improvement in the value of coronal temperature is found.

Detection of Singly Ionized Oxygen Around Jupiter

Science ◽  
1979 ◽  
Vol 205 (4403) ◽  
pp. 297-298 ◽  
Author(s):  
C. B. PILCHER ◽  
J. S. MORGAN
Keyword(s):  
Line Intensity ◽  
Intensity Ratio ◽  
Magnetic Equator ◽  
Jovian Magnetosphere ◽  
Line Intensity Ratio ◽  
Sulfur Emission ◽  
Plasma Characteristics

Forbidden emission from singly ionized oxygen at wavelengths of 3726 and 3729 angstroms has been detected in the inner Jovian magnetosphere. The emission is present between ∼4 and ∼7 to 8 Jovian radii from the planet and appears concentrated in the magnetic equator. The line intensity ratio indicates the same plasma characteristics as those derived from observations of forbidden sulfur emission.

Complex Variations in the Line-Intensity Ratio of Coronal Emission Lines with Height above the Limb

2004 ◽  
Vol 617 (1) ◽  
pp. L81-L84 ◽  
Author(s):  
Jagdev Singh ◽  
Takashi Sakurai ◽  
Kiyoshi Ichimoto ◽  
Tetsuya Watanabe
Keyword(s):  
Line Intensity ◽  
Intensity Ratio ◽  
Emission Lines ◽  
Coronal Emission ◽  
Line Intensity Ratio
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