Enhanced red emission in ZnMoO4 : Eu3+by charge compensation

2010 ◽  
Vol 43 (5) ◽  
pp. 055101 ◽  
Author(s):  
An Xie ◽  
Ximing Yuan ◽  
Fengxiang Wang ◽  
Yu Shi ◽  
Zhongfei Mu
2014 ◽  
Vol 62 ◽  
pp. 63-68 ◽  
Author(s):  
Zhi-wei Zhang ◽  
Ya-nan Wu ◽  
Xi-hai Shen ◽  
Yan-jun Ren ◽  
Wei-guo Zhang ◽  
...  

2022 ◽  
Vol 241 ◽  
pp. 118504
Author(s):  
Zhongxu Han ◽  
Shuchen Lü ◽  
Qingyu Meng ◽  
Mengsi Sun ◽  
Yandong Ren

2019 ◽  
Vol 214 ◽  
pp. 116569 ◽  
Author(s):  
Jiahui Chen ◽  
Yujun Liang ◽  
Yingli Zhu ◽  
Shiqi Liu ◽  
Haoran Li ◽  
...  

2014 ◽  
Vol 12 (5) ◽  
pp. 051602-51605 ◽  
Author(s):  
Hongling Yu Hongling Yu ◽  
Xue Yu Xue Yu ◽  
Xuhui Xu Xuhui Xu ◽  
Qing Jiao Qing Jiao ◽  
Tingming Jiang Tingming Jiang ◽  
...  

2011 ◽  
Vol 34 (1) ◽  
pp. 89-94 ◽  
Author(s):  
Zhongfei Mu ◽  
Yihua Hu ◽  
Li Chen ◽  
Xiaojuan Wang

2014 ◽  
Vol 35 (9) ◽  
pp. 1071-1075 ◽  
Author(s):  
张志伟 ZHANG Zhi-wei ◽  
王晓娟 WANG Xiao-juan ◽  
任艳军 REN Yan-jun

2011 ◽  
Vol 158 (10) ◽  
pp. J287 ◽  
Author(s):  
Zhongfei Mu ◽  
Yihua Hu ◽  
Li Chen ◽  
Xiaojuan Wang

1994 ◽  
Vol 144 ◽  
pp. 597-599 ◽  
Author(s):  
I. V. Alexeyeva ◽  
N. L. Kroussanova ◽  
M. V. Streltsova

AbstractThe results of photometry of colour positives of the solar corona of July 11, 1991 are presented. Observations of the white corona were made without radial niters in Jojutla (Mexico). Dependences of coronal brightness on distance in the red (640 nm) and blue (420 nm) wavelength intervals are deduced for different coronal structures up to 3.0-3.5R⊙. The effect of ”reddening“ is noted. The excess of the red emission to the blue one (I640nm/I420nm) is found to be 1.20 and 1.17 at distance of 2.2R⊙for the N-E helmet streamer (P ≃ 37°) and the N-W region of low brightness (P ≃ 339°), respectively.


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