Study on Mid-Infrared Spectral Properties of Ho3+/Yb3+Co-Doped Fluorogermanate Glasses

2016 ◽  
Vol 36 (6) ◽  
pp. 0616002
Author(s):  
钱国权 Qian Guoquan ◽  
唐国武 Tang Guowu ◽  
钱奇 Qian Qi ◽  
陈敢新 Chen Ganxin
2018 ◽  
Vol 8 (12) ◽  
pp. 3820 ◽  
Author(s):  
Zhen Zhang ◽  
Fengkai Ma ◽  
Xinsheng Guo ◽  
Jingya Wang ◽  
Xiaobo Qian ◽  
...  

2010 ◽  
Vol 717 (2) ◽  
pp. 868-877 ◽  
Author(s):  
D. Farrah ◽  
T. Urrutia ◽  
M. Lacy ◽  
V. Lebouteiller ◽  
H. W. W. Spoon ◽  
...  

Sensors ◽  
2021 ◽  
Vol 21 (6) ◽  
pp. 2155
Author(s):  
Marcin Kochanowicz ◽  
Jacek Zmojda ◽  
Agata Baranowska ◽  
Marta Kuwik ◽  
Bartłomiej Starzyk ◽  
...  

This work reports on the fabrication and analysis of near-infrared and mid-infrared luminescence spectra and their decays in fluoroindate glasses co-doped with Yb3+/Ho3+. The attention has been paid to the analysis of the Yb3+→ Ho3+ energy transfer processed ions in fluoroindate glasses pumped by 976 nm laser diode. The most effective sensitization for 2 μm luminescence has been obtained in glass co-doped with 0.8YbF3/1.6HoF3. Further study in the mid-infrared spectral range (2.85 μm) showed that the maximum emission intensity has been obtained in fluoroindate glass co-doped with 0.1YbF3/1.4HoF3. The obtained efficiency of Yb3+→ Ho3+ energy transfer was calculated to be up to 61% (0.8YbF3/1.6HoF3), which confirms the possibility of obtaining an efficient glass or glass fiber infrared source for a MID-infrared (MID-IR) sensing application.


2008 ◽  
Author(s):  
X. Y. Xia ◽  
C. Cao ◽  
S. Mao ◽  
Z. G. Deng ◽  
Da-Shin Lee ◽  
...  

2011 ◽  
Vol 42 (17) ◽  
pp. 2143-2159 ◽  
Author(s):  
Francisco J. Calderón ◽  
Maysoon M. Mikha ◽  
Merle F. Vigil ◽  
David C. Nielsen ◽  
Joseph G. Benjamin ◽  
...  

2013 ◽  
Vol 772 (1) ◽  
pp. 28 ◽  
Author(s):  
Peng Wei ◽  
Zhaohui Shang ◽  
Michael S. Brotherton ◽  
Sabrina L. Cales ◽  
Dean C. Hines ◽  
...  

1999 ◽  
Vol 194 ◽  
pp. 54-59
Author(s):  
O. Laurent ◽  
I.F. Mirabel

We present a new diagnostic tool based on mid-infrared spectra (5–16μm) for distinguishing the emission triggered by the active galactic nucleus (AGN) and by the star formation activity. We show that the AGN spectra, contrary to the starburst spectra, present an important continuum below 9μm and an absence of Unidentified Infrared Bands (UIBs).


2012 ◽  
Vol 755 (1) ◽  
pp. 29 ◽  
Author(s):  
Mariana S. Lazarova ◽  
Gabriela Canalizo ◽  
Mark Lacy ◽  
Anna Sajina

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