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Study on Novel Topology of Solar–Wind Hybrid Power Plant Using Photovoltaic Cell Emulating System
Vu Minh Phap,N. Yamamura,M. Ishida,Nguyen Thuy Nga,I. Mizoguchi,T. Yamashita 대한전기학회 2019 Journal of Electrical Engineering & Technology Vol.14 No.2
At the present, the grid-tied solar power system is the most promising as a renewable energy technology for replacing the fossil energy sources. The usage effi ciency of the power conditioner system in the grid-tied solar power system is not high because the electricity generation from solar panels depends on the weather. The utilization rate of the power conditioner system can be increased by adding the small scale wind turbine to the existing grid-tied solar power system. We introduced a novel design solution in the previous study to connect the small wind turbine with the power conditioner system of the grid-tied solar power system by emulating technical characteristics of the solar panel in series connection mode. By which, the utilization rate of the power conditioner system has been increased. However, this improved utilization rate of the power conditioner system is not high in the cloudy and rainy days because the voltage of the solar panel changes slightly and the maximum input voltage of the power conditioner system is limited. Therefore, we propose a novel performance enhancement method for solar–wind hybrid power plant using photovoltaic cell emulating system in this research.
Chris Sedgwick,STEPHEN SERJEANT,CHRIS PEARSON,I. Yamamura,S. Makiuti,N. Ikeda,Y. Fukuda,S. Oyabu,T. Koga,S. Amber,Glenn J. White 한국천문학회 2017 天文學論叢 Vol.32 No.1
We have identified 22 quasars in the AKARI far-infrared all-sky Bright Source Catalogue, using a matching radius of < 10 “, and excluding matches which are close to foreground extended sources or cirrus. We have confirmed a relation between quasar optical luminosity and far-infrared luminosity which was found in an earlier study. In addition, we have found that the 11 sources which are at redshift z > 1 are magnified with respect to the predicted far-infrared luminosity, and consider this may be due to gravitational lensing. If confirmed, this would provide a new way to identify lenses; if not, we may have identified an interesting new population of extreme starbursting quasars. %We are currently seeking spectroscopic confirmation of the redshifts and improved imaging for these sources.
Matsuta, K.,Gandhi, P.,Dotani, T.,Nakagawa, T.,Isobe, N.,Ueda, Y.,Ichikawa, K.,Terashima, Y.,Oyabu, S.,Yamamura, I.,Stawarz, L. The Korean Astronomical Society 2012 天文學論叢 Vol.27 No.4
We combine data from two all-sky surveys, the Swift/Burst Alert Telescope 22 Month Source Catalog and the AKARI Point Source Catalogue, in order to study the connection between the hard X-ray (> 10 keV) and infrared (IR) properties of local active galactic nuclei (AGN). We find two photometric diagnostics are useful for source classification: one is the X-ray luminosity vs. IR color diagram, in which type 1 radio-loud AGN are well isolated from other AGN. The second one uses the X-ray vs. IR color-color diagram as a redshift-independent indicator for identifying Compton-thick (CT) AGN. Importantly, CT AGN and starburst galaxies in composite systems can also be separated in this plane based upon their hard X-ray fluxes and dust temperatures. This diagram may be useful as a new indicator to classify objects in new surveys such as with WISE and NuSTAR.