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A Study of 10 MHz Multi-Sampling SVPWM method for Three Phase Inverter using USPM Controller
S. Takeuchi,K. Sato,T. Yokoyama 전력전자학회 2023 ICPE(ISPE)논문집 Vol.2023 No.-
In the development process of power electronics system, a wide range of know-how is required for special purpose circuits such as main circuits, control circuits and gate drive circuits. The Universal Smart Power Module (USPM) has been proposed to solve these problems by converting the above circuits into one module to reduce the design cost and development time. To realize the USPM module, USPM controller was developed which has very high speed A/D converter and high specification SoC-FPGA chip, ultra high speed control calculation can be realized. In this paper, a new space vector PWM (SVPWM) method that improves the transient response and robustness by 10MHz sampling between carriers and compensating the output vector in real time. The output vector is recalculated in every 0.1us by using USPM controller, and the recalculation immediately reflected to the output vector, which improves the output characteristics of three phase inverter. The advantage of high speed sampling digital feedback method are verified.
DETECTION OF THE COSMIC FAR-INFRARED BACKGROUND IN AKARI DEEP FIELD SOUTH
Matsuura, S.,Shirahata, M.,Kawada, M.,Takeuchi, T. T.,Burgarella, D.,Clements, D. L.,Jeong, W.-S.,Hanami, H.,Khan, S. A.,Matsuhara, H.,Nakagawa, T.,Oyabu, S.,Pearson, C. P.,Pollo, A.,Serjeant, S.,Taka IOP Publishing 2011 The Astrophysical journal Vol.737 No.1
<P>We report new limits on the absolute brightness and spatial fluctuations of the cosmic infrared background (CIB) via the AKARI satellite. We carried out observations at 65, 90, 140, and 160 mu m as a cosmological survey in AKARI Deep Field South, which is one of the lowest cirrus regions with a contiguous area of the sky. After removing bright galaxies and subtracting zodiacal and Galactic foregrounds from the measured sky brightness, we successfully measured the CIB brightness and its fluctuations across a wide range of angular scales, from arcminutes to degrees. The measured CIB brightness is consistent with previous results reported from COBE data, but significantly higher than the lower limits at 70 and 160 mu m obtained via Spitzer from the stacking analysis of selected 24 mu m sources. The discrepancy with the Spitzer result is possibly due to a new galaxy population at high redshift obscured by hot dust or unknown diffuse emission. From a power spectrum analysis at 90 mu m, two components were identified: the CIB fluctuations with shot noise due to individual galaxies in a small angular scale from the beam size up to 10 arcminutes, and Galactic cirrus emission dominating at the largest angular scales of a few degrees. The overall shape of the power spectrum at 90 mu m is very similar to that at longer wavelengths, as observed by Spitzer and the Balloon-borne Large-Aperture Submillimeter Telescope (BLAST). Our power spectrum, with an intermediate angular scale of 10-30 arcminutes, gives a firm upper limit for galaxy clustering, which was found by Spitzer and BLAST. Moreover, the color of the CIB fluctuations, which is obtained by combining our data with the previous results, is as red as ultra-luminous infrared galaxies at high redshift. These galaxies are not likely to provide the majority of the CIB emission at 90 mu m, but are responsible for the fluctuations. Our results provide new constraints on the evolution and clustering properties of distant infrared galaxies and any diffuse emission from the early universe.</P>
Origin of the ferromagnetism in ZnCoO from chemical reaction of Co<sub>3</sub>O<sub>4</sub>
Lee, S.,Kim, B.S.,Chan Cho, Y.,Shin, J.M.,Seo, S.W.,Cho, C.R.,Takeuchi, I.,Jeong, S.Y. Elsevier 2013 Current Applied Physics Vol.13 No.9
We investigated conversion of Co<SUB>3</SUB>O<SUB>4</SUB> to Co nanoclusters through hydrogen reduction. Quantitative analysis is performed on the conversion of Co<SUB>3</SUB>O<SUB>4</SUB> to Co metal as a function of hydrogen-injection conditions. Our results reveal that Co<SUB>3</SUB>O<SUB>4</SUB> must be completely eliminated to avoid formation of the metal phase in ZnCoO. We also propose a new M-T curve based method for detecting nano-sized Co clusters which are below the detection limit of diffraction techniques. It is also found that the Co phase can be transformed back to the Co<SUB>3</SUB>O<SUB>4</SUB> phase through oxygen annealing and that, as a result, the ferromagnetism can be eliminated. These findings are discussed in the context of the origin of ferromagnetism in ZnCoO.
Invariant Mass Spectroscopy for the Neutron Rich Nuclei
사토,추경호,방형찬,S. H. Choi,T. Nakamura,Y. Kondo,Y. Nakayama,N. Kobayashi,K. N. Tanaka,S. Deguchi,Y. Kawada,N. Tanaka,T. Sugimoto,T. Motobayashi,H. Sakurai,H. Otsu,N. Aoi,Y. Yanagisawa,S. Takeuchi,N. Fukuda 한국물리학회 2011 THE JOURNAL OF THE KOREAN PHYSICAL SOCIETY Vol.59 No.23
The neutron-rich carbon isotopes ^(19,17)C and a boron isotope ^(14)B are investigated respectively via proton inelastic and charge-exchange reactions on a liquid hydrogen target at around 70 MeV/nucleon at RIKEN. The invariant mass method in inverse kinematics involving coincidence detection of a charged fragment and a neutron both emitted at forward angles is employed to map the energy spectrum above the neutron decay threshold. Several resonance structures are revealed in the invariant mass spectra, and the nature for some of them is discussed from comparisons of differential cross section data with predictions of microscopic DWBA calculations based on spsdpf shell model wave functions and a recent parametrization of semi-microscopic nucleon-nucleus optical model potential (JLMB). By extrapolating the (p,n) cross sections leading to the 1^+ state at 1.27 MeV in ^(141)B to zero momentum transfer the Gamow-Teller transition strength is deduced. The value is found to compare well with that reported in a β-delayed neutron emission study.
OVERVIEW OF THE NORTH ECLIPTIC POLE DEEP MULTI-WAVELENGTH SURVEY (NEP-DEEP)
Matsuhara, H.,Wada, T.,Takagi, T.,Nakagawa, T.,Murata, K.,Churei, S.,Goto, T.,Oyabu, S.,Takeuchi, T.T.,Ohyama, Y.,Miyaji, T.,Krumpe, M.,Lee, H.M.,Im, M.,Serjeant, S.,Peason, C.P.,White, G.,Malkan, M.A The Korean Astronomical Society 2012 天文學論叢 Vol.27 No.4
An overview of the North Ecliptic Pole (NEP) deep multi-wavelength survey covering from X-ray to radio wavelengths is presented. The main science objective of this multi-wavelength project is to unveil the star-formation and AGN activities obscured by dust in the violent epoch of the Universe (z=0.5-2), when the star formation and black-hole evolution activities were much stronger than the present. The NEP deep survey with AKARI/IRC consists of two survey projects: shallow wide (8.2 sq. deg, NEP-Wide) and the deep one (0.6 sq. deg, NEP-Deep). The NEP-Deep provides us with a $15{\mu}m$ or $18{\mu}m$ selected sample of several thousands of galaxies, the largest sample ever made at these wavelengths. A continuous filter coverage at mid-IR wavelengths (7, 9, 11, 15, 18, and $24{\mu}m$) is unique and vital to diagnose the contribution from starbursts and AGNs in the galaxies at the violent epoch. The recent updates of the ancillary data are also provided: optical/near-IR magnitudes (Subaru, CFHT), X-ray (Chandra), FUV/NUV (GALEX), radio (WSRT, GMRT), optical spectra (Keck/DEIMOS etc.), Subaru/FMOS, Herschel/SPIRE, and JCMT/SCUBA-2.
Li, H.,Kilpelä,inen, T. O.,Liu, C.,Zhu, J.,Liu, Y.,Hu, C.,Yang, Z.,Zhang, W.,Bao, W.,Cha, S.,Wu, Y.,Yang, T.,Sekine, A.,Choi, B. Y.,Yajnik, C. S.,Zhou, D.,Takeuchi, F.,Yamamoto, K.,Chan, J. C.,Man Springer-Verlag 2012 Diabetologia Vol.55 No.4
<P><B>Aims/hypothesis</B></P><P><I>FTO</I> harbours the strongest known obesity-susceptibility locus in Europeans. While there is growing evidence for a role for <I>FTO</I> in obesity risk in Asians, its association with type 2 diabetes, independently of BMI, remains inconsistent. To test whether there is an association of the <I>FTO</I> locus with obesity and type 2 diabetes, we conducted a meta-analysis of 32 populations including 96,551 East and South Asians.</P><P><B>Methods</B></P><P>All studies published on the association between <I>FTO</I>-rs9939609 (or proxy [<I>r</I><SUP>2</SUP> > 0.98]) and BMI, obesity or type 2 diabetes in East or South Asians were invited. Each study group analysed their data according to a standardised analysis plan. Association with type 2 diabetes was also adjusted for BMI. Random-effects meta-analyses were performed to pool all effect sizes.</P><P><B>Results</B></P><P>The <I>FTO</I>-rs9939609 minor allele increased risk of obesity by 1.25-fold/allele (<I>p</I> = 9.0 × 10<SUP>−19</SUP>), overweight by 1.13-fold/allele (<I>p</I> = 1.0 × 10<SUP>−11</SUP>) and type 2 diabetes by 1.15-fold/allele (<I>p</I> = 5.5 × 10<SUP>−8</SUP>). The association with type 2 diabetes was attenuated after adjustment for BMI (OR 1.10-fold/allele, <I>p</I> = 6.6 × 10<SUP>−5</SUP>). The <I>FTO</I>-rs9939609 minor allele increased BMI by 0.26 kg/m<SUP>2</SUP> per allele (<I>p</I> = 2.8 × 10<SUP>−17</SUP>), WHR by 0.003/allele (<I>p</I> = 1.2 × 10<SUP>−6</SUP>), and body fat percentage by 0.31%/allele (<I>p</I> = 0.0005). Associations were similar using dominant models. While the minor allele is less common in East Asians (12–20%) than South Asians (30–33%), the effect of <I>FTO</I> variation on obesity-related traits and type 2 diabetes was similar in the two populations.</P><P><B>Conclusions/interpretation</B></P><P><I>FTO</I> is associated with increased risk of obesity and type 2 diabetes, with effect sizes similar in East and South Asians and similar to those observed in Europeans. Furthermore, <I>FTO</I> is also associated with type 2 diabetes independently of BMI.</P><P><B>Electronic supplementary material</B></P><P>The online version of this article (doi:10.1007/s00125-011-2370-7) contains peer-reviewed but unedited supplementary material, which is available to authorised users.</P>