scholarly journals Wave Activity in Jupiter's North Equatorial Belt From Near‐Infrared Reflectivity Observations

2019 ◽  
Vol 46 (3) ◽  
pp. 1232-1241 ◽  
Author(s):  
Rohini S. Giles ◽  
Glenn S. Orton ◽  
Andrew W. Stephens ◽  
Michael H. Wong ◽  
Patrick G. J. Irwin ◽  
...  
2018 ◽  
Vol 229 ◽  
pp. 171-173 ◽  
Author(s):  
Yu Chen ◽  
Yan Ma ◽  
Zhoufu Wang ◽  
Xitang Wang ◽  
Hao Liu ◽  
...  

1983 ◽  
Vol 43 (12) ◽  
pp. 1093-1095 ◽  
Author(s):  
R. B. Goldner ◽  
D. H. Mendelsohn ◽  
J. Alexander ◽  
W. R. Henderson ◽  
D. Fitzpatrick ◽  
...  

RSC Advances ◽  
2019 ◽  
Vol 9 (66) ◽  
pp. 38822-38827
Author(s):  
Ryohei Oka ◽  
Senri Iwasaki ◽  
Toshiyuki Masui

The near infrared reflectivity and black color tone of a Ca2Mn0.85Ti0.15O4 pigment were improved by the introduction of strain with Zn2+ doping into the [MnO6] octahedra and a decrease in the manganese ion concentration.


2011 ◽  
Vol 121-126 ◽  
pp. 3960-3964
Author(s):  
Jing Chang Zhuge ◽  
Zhi Jing Yu ◽  
Jian Shu Gao

In order to detect the ice on aircraft wings, a method based on near infrared image processing is proposed. According to the variety of near-infrared reflectivity, four images of one object are obtained under different detection wavelengths. Water and ice can be distinguished by the different variation trends of near infrared images. In this paper, 1.10μm, 1.16μm, 1.26μm and 1.28μm are selected to be the detection wavelengths. The images of Carbon Fiber Composite material aircraft wings partially covered by water or ice are obtained and analyzed. Parameter D can reflect the variation trend of relative near-infrared reflectivity, so that Parameter D also can be the distinguish basis. The results of the experiment show that the method proposed in this paper is available for ice detection.


2019 ◽  
Vol 45 (11) ◽  
pp. 14198-14204
Author(s):  
Xiaotong Jin ◽  
Kangkang Yuan ◽  
Yongshuai Xie ◽  
Chonghe Xu ◽  
Lin Wang ◽  
...  

2012 ◽  
Vol 107 (3) ◽  
pp. 669-673 ◽  
Author(s):  
S. W. Shu ◽  
J. Zhang ◽  
C. K. Tsang ◽  
L. G. Shi ◽  
Y. Y. Li

2017 ◽  
Vol 44 (14) ◽  
pp. 7140-7148 ◽  
Author(s):  
L. N. Fletcher ◽  
G. S. Orton ◽  
J. A. Sinclair ◽  
P. Donnelly ◽  
H. Melin ◽  
...  

1998 ◽  
Vol 103 (E10) ◽  
pp. 23023-23041 ◽  
Author(s):  
M. Roos-Serote ◽  
P. Drossart ◽  
T. Encrenaz ◽  
E. Lellouch ◽  
R. W. Carlson ◽  
...  

2021 ◽  
Vol 121 ◽  
pp. 111517
Author(s):  
Tao Liang ◽  
Gang Peng ◽  
Xiangzhe Zhang ◽  
Yuehua Wei ◽  
Xiaoming Zheng ◽  
...  

2018 ◽  
Vol 4 (2) ◽  
pp. 109-115
Author(s):  
Вера Сивцева ◽  
Vera Sivtseva ◽  
Петр Аммосов ◽  
Petr Ammosov ◽  
Галина Гаврильева ◽  
...  

Since 2015, simultaneous observations of temperature of the high-latitude mesopause (87 km) have been made at Maimaga (63.04° N, 129.51° E) and Tiksi (71.58° N, 128.77° E) stations. These stations record spectra with Shamrock (Andor) photosensitive infrared spectrographs detecting the OH (3, 1) band in the near-infrared region (about 1.5 μm). We analyze temperature data obtained in observation seasons from 2015 to 2017. Standard deviations of temperature σ from its mean values are taken as characteristics of wave activity at night. We have obtained standard temperature deviations corresponding to internal gravity waves (IGW) (σgw) and tidal waves (σtd). Mean night rotational temperatures of hydroxyl emission almost coincide, and seasonal variations of gravity and tidal waves have a similar form during two seasons of simultaneous observations at Tiksi and Maimaga.


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