Leveraging a New Energy Source to Enhance Heavy Oil and Oilsands Production

2005 ◽  
Author(s):  
Cameron James Geddes ◽  
Harry Bailey Curlett
Keyword(s):  
2014 ◽  
Vol 962-965 ◽  
pp. 1787-1791
Author(s):  
Qiu Yue Li ◽  
Jie Ping Han

The new energy power generation in China has rapidly developed, and many generation companies have invested in new energy source. Some projects cannot achieve the desired results as the characters as dispersion, instability, and low level of technique. This article has established the index system of the risk degree for new energy power generation, which included the the risk degree of politics, economy, technology, environment, management. And making the analysis of the risk factors, it can provide the significant meaning of the investment for the new energy power generation companies.


2015 ◽  
Vol 733 ◽  
pp. 680-683
Author(s):  
Ya Rong He

Sustainable exploration and use of energy source depend on discovery of new energy source and development of novel energy devices. As a kind of energy storage device, supercapacitors have many advantages over conventional batteries: high power density, long cycling stability, fast charge-discharge rate and being environment friendly. However, common problems involved with nanomaterials such as bad structural continuity, conglomeration and structural instability have restricted their application in supercapacitors. We have conducted the design, synthesis and performance research of the electrode materials containing. We demonstrate the above composite materials have wide prospect for application in the supercapacitors as well as other similar fields.


2016 ◽  
Vol 100 ◽  
pp. 484-491 ◽  
Author(s):  
K. Malak ◽  
C. de la Seiglière ◽  
C. Fernández ◽  
M. Swaminathan ◽  
A. Sebastián ◽  
...  
Keyword(s):  

1982 ◽  
Vol 97 ◽  
pp. 69-70
Author(s):  
David S. De Young

In addition to the occurrence of emission line regions coexistent with extended radio sources which have been discussed at this Symposium, this phenomenon has been observed earlier in 3C277.3 (Miley et al. 1981) and in Centaurus A (Graham and Price 1981). This gas has been detected only in the Fanaroff and Riley “Class I” radio sources. Data concerning this class of object suggest that outflow from the nucleus is proceeding at transonic or subsonic speeds and this correlation has led to the suggestion (De Young 1981) that the origin of the emission line gas arises from entrainment of the interstellar medium into the ejected material.


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