Self-Modeling Curve Resolution Study of Temperature-Dependent Near-Infrared Spectra of Water and the Investigation of Water Structure

2002 ◽  
Vol 106 (5) ◽  
pp. 760-766 ◽  
Author(s):  
S. Šašić ◽  
V. H. Segtnan ◽  
Y. Ozaki
Keyword(s):  
Infrared Spectra ◽  
Near Infrared ◽  
Water Structure ◽  
Temperature Dependent ◽  
Curve Resolution ◽  
Near Infrared Spectra ◽  
Resolution Study

Glucose induced variation of water structure from temperature dependent near infrared spectra

RSC Advances ◽  
2016 ◽  
Vol 6 (107) ◽  
pp. 105729-105736 ◽  
Author(s):  
Xiaoyu Cui ◽  
Wensheng Cai ◽  
Xueguang Shao
Keyword(s):  
Aqueous Solutions ◽  
Infrared Spectra ◽  
Near Infrared ◽  
Water Structure ◽  
Temperature Dependent ◽  
Near Infrared Spectra ◽  
Induced Variation ◽  
Water Species

The different effects of glucose on water species provide evidence to explain the bioprotective function of carbohydrates in aqueous solutions.

Multilevel analysis of temperature dependent near-infrared spectra

Talanta ◽  
2015 ◽  
Vol 131 ◽  
pp. 170-174 ◽  
Author(s):  
Ruifeng Shan ◽  
Yue Zhao ◽  
Mengli Fan ◽  
Xiuwei Liu ◽  
Wensheng Cai ◽  
...  
Keyword(s):  
Multilevel Analysis ◽  
Infrared Spectra ◽  
Near Infrared ◽  
Temperature Dependent ◽  
Near Infrared Spectra

Water can be a probe for sensing glucose in aqueous solutions by temperature dependent near infrared spectra

2017 ◽  
Vol 957 ◽  
pp. 47-54 ◽  
Author(s):  
Xiaoyu Cui ◽  
Xiuwei Liu ◽  
Xiaoming Yu ◽  
Wensheng Cai ◽  
Xueguang Shao
Keyword(s):  
Aqueous Solutions ◽  
Infrared Spectra ◽  
Near Infrared ◽  
Temperature Dependent ◽  
Near Infrared Spectra

scholarly journals Near infrared spectra of O stars and related objects

1979 ◽  
Vol 83 ◽  
pp. 131-137
Author(s):  
J.M. Vreux ◽  
Y. Andrillat
Keyword(s):  
Infrared Spectra ◽  
Near Infrared ◽  
Favorable Condition ◽  
Temperature Dependent ◽  
Near Infrared Spectra ◽  
Theoretical Predictions

The λ 10124 He II line has been found to be a measurable emission in three stars. Our new data are compared to theoretical predictions. The λ 10830 He I line is observed in emission in 74% of the 05–08 supergiants but only seen in 29 % of the dwarfs, all of the latter exhibiting some “pecularities” i.e. classified as Oef, Oe, ON or On. An envelope with a sufficient amount of material seems to be a favorable condition to get the λ 10830 line in emission. However the mechanism leading to the observed emission is temperature dependent as well.

Sign in / Sign up

Export Citation Format

Share Document