scholarly journals A halation reduction method for high quality images of tomato fruits in greenhouse

2015 ◽  
Vol 8 (4) ◽  
pp. 200-206 ◽  
Author(s):  
Xiao Cheng ◽  
Naoshi Kondo ◽  
Yuichi Ogawa ◽  
Tomoo Shiigi ◽  
Slamet Widodo ◽  
...  
2012 ◽  
Vol 557-559 ◽  
pp. 1539-1542
Author(s):  
Jian Fang Wang ◽  
Ya Nan Lv ◽  
Yin Long ◽  
Cheng An Tao ◽  
Hui Zhu

In this paper, the graphene oxide reducing by photochemical-thermal reduction and high-temperature thermal reduction was studied to get qualified graphene and avoid the re-aggregation. The results show that graphene obtained by both of the two reduction methods all maintained the original well-layered morphology of the graphene oxide. The graphene had smooth surface and high quality as completely reduced by high-temperature thermal method. However, the reduction the photochemical-thermal reaction was not sufficient and caused many vesicles on the graphene surface due to the low temperature and the lack of reaction time.


2012 ◽  
Vol 711 ◽  
pp. 91-98 ◽  
Author(s):  
Hiroyuki Nagasawa ◽  
Takamitsu Kawahara ◽  
Kuniaki Yagi ◽  
Naoki Hatta ◽  
Hidetsugu Uchida ◽  
...  

Quantitative efficacies of several methods for stacking fault (SF) reduction are evaluated using Monte Carlo (MC) simulation. SF density on a 3C–SiC {001} surface depends on interactions of adjoining SFs: annihilation between counter pairs of SFs and termination by orthogonal SF pairs. However, SFs are not entirely eliminated when growth occurs on undulant-Si and switch back epitaxy (SBE) due to spontaneous SF collimation that suppresses the annihilation probability of counter SFs. The MC simulation also reveals the efficacy of SF reduction method which includes the growth of 3C–SiC on finite area bounded by side walls. One can theoretically reduce the SF density below 100 cm-1on 3C–SiC {001} surface. A practical way for eliminating the SF by termination at side walls is demonstrated, and it clearly exhibits that the SF density can be reduced under 120 cm-1.


2020 ◽  
Vol 8 (40) ◽  
pp. 21062-21069
Author(s):  
Mei Han ◽  
Yongjie Ge ◽  
Jianfang Liu ◽  
Zhongzhong Cao ◽  
Moxia Li ◽  
...  

A novel mixed PVP hydrogel-mediated polyol reduction method was developed for the synthesis of high-quality Ag nanowires with negligible Ag nanoparticles produced, high aspect ratio (exceeding 1200), and a thin (∼1 nm) capping layer.


2018 ◽  
Vol 6 (7) ◽  
pp. 1829-1835 ◽  
Author(s):  
Wen-Shuai Jiang ◽  
Chao Yang ◽  
Guo-Xing Chen ◽  
Xiao-Qing Yan ◽  
Shao-Nan Chen ◽  
...  

High-quality intrinsic graphene can be prepared by a simple triggered microwave reduction method under air conditions, which provides a simple and low-cost route for large-scale production of high-quality graphene.


2013 ◽  
Vol 27 (19) ◽  
pp. 1341005
Author(s):  
YUHONG ZHANG ◽  
BIAO YAN ◽  
WEI LU

Graphite oxide was prepared by Hummers method, then it was obtained by ultrasound. Finally, graphene was prepared by using hydrazine hydrate as reducing agent. We can get the influences of oxidation time on the graphene structure by different reacting times. Ultrasonication can reduce the aggregation of graphene efficiently. The morphology and size of graphene were characterized by SEM, TEM, XRD and FTIR. Through this method, we can get high quality graphene which has smooth surface and fewer defects. The longer the oxidation time, the more easier it is to peel and insert functional groups.


2019 ◽  
Vol 45 (18) ◽  
pp. 23954-23965 ◽  
Author(s):  
Shanshan Kang ◽  
Jinyang Zhuang ◽  
Shaohong Kang ◽  
Yan Peng ◽  
Shiyou Guan

1966 ◽  
Vol 24 ◽  
pp. 51-52
Author(s):  
E. K. Kharadze ◽  
R. A. Bartaya

The unique 70-cm meniscus-type telescope of the Abastumani Astrophysical Observatory supplied with two objective prisms and the seeing conditions characteristic at Mount Kanobili (Abastumani) permit us to obtain stellar spectra of a high quality. No additional design to improve the “climate” immediately around the telescope itself is being applied. The dispersions and photographic magnitude limits are 160 and 660Å/mm, and 12–13, respectively. The short-wave end of spectra reaches 3500–3400Å.


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