scholarly journals ON THE NATURE OF THE FLAME EMISSION SPECTRUM OF CRUDE OIL BLAZE AT BAGHJAN

2020 ◽  
Vol 8 (8) ◽  
pp. 574-578
Author(s):  
R. Konwar ◽  
◽  
R. Mahanta ◽  
J. Saikia ◽  
S. Konwar ◽  
...  
1952 ◽  
Vol 20 (11) ◽  
pp. 1808-1809 ◽  
Author(s):  
B. W. Bullock ◽  
C. E. Feazel ◽  
P. Gloersen ◽  
S. Silverman

1954 ◽  
Vol 52 (3) ◽  
pp. 161 ◽  
Author(s):  
W.S. Benedict ◽  
A.M. Bass ◽  
E.K. Plyler

1988 ◽  
Vol 14 (6) ◽  
pp. 713-720 ◽  
Author(s):  
Masakazu Yamazaki ◽  
Masaaki Ohya ◽  
Kentaro Tsuchiya

2011 ◽  
Vol 48 (5) ◽  
pp. 053001
Author(s):  
许凌飞 Xu Lingfei ◽  
李武森 Li Wusen ◽  
陈延如 Chen Yanru ◽  
徐实学 Xu Shixue ◽  
李伽 Li Jia ◽  
...  

2020 ◽  
Vol 204 ◽  
pp. 106423 ◽  
Author(s):  
Shu Zheng ◽  
Yu Yang ◽  
Xinyu Li ◽  
Huawei Liu ◽  
Weijie Yan ◽  
...  

2011 ◽  
Vol 55-57 ◽  
pp. 16-19
Author(s):  
Ling Fei Xu ◽  
Wu Sen Li ◽  
Shi Xue Xu ◽  
Jia Li ◽  
Yong Qing Wang

The flame of basic oxygen furnace is the most important evident in the steel making process. This studies dividing the flame’s spectrum into two parts: the background spectrum and the characteristic atomic emission spectrum. Compared the figure of the characteristic atomic emission spectrum measured by spectrometer with the Gaussian function, the conclusion shows that the background spectrum could compensate the loss of the light intensity which due to the stimulated absorption of characteristic atomic. Based on the FES ( flame emission spectrometer) and spectrum in the BOF’s flame, the studies deduce a new relationship between the intensity of characteristic atomic spectrum and the temperature of the flame. The results indicates that the temperature measured by FES is inosculated to the temperature obtained by converter sublance comparatively.


1979 ◽  
Vol 44 ◽  
pp. 349-355
Author(s):  
R.W. Milkey

The focus of discussion in Working Group 3 was on the Thermodynamic Properties as determined spectroscopically, including the observational techniques and the theoretical modeling of physical processes responsible for the emission spectrum. Recent advances in observational techniques and theoretical concepts make this discussion particularly timely. It is wise to remember that the determination of thermodynamic parameters is not an end in itself and that these are interesting chiefly for what they can tell us about the energetics and mass transport in prominences.


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