• 제목/요약/키워드: dV/dt

검색결과 42건 처리시간 0.024초

$SF_6-N_2$ 혼합가스에서 과도임펄스전압에 대한 V-t특성 (V-t Characteristics in $SF_6-N_2$ Mixtures for Transient Impulse Voltages)

  • 이복희;이경옥
    • 대한전기학회논문지:전기물성ㆍ응용부문C
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    • 제50권9호
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    • pp.456-465
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    • 2001
  • In this paper, breakdown voltages in $SF_6-N_2$ mixtures were experimentally investigated to understand characteristics of dielectric strength and physical phenomena in nonuniform field disturbed by a needle shape protrusion. The test voltages are the lightning impulse$(\pm1.2/44 \mus)$ and the damped oscillatory impulse$(\pm400 ns / 0.83 MHz)$ voltages which can be occurred by the operation of disconnecting switches in gas-insulated switchgears(GIS). The effects of the polarity and wave shape of the test voltages, and the gas pressure on the V-t characteristics were in detail examined. The V-t characteristic curves were measured in different two ways : (1) one is the method by taking the maximum voltage recorded at or prior to breakdown against the time to breakdown, that is, the Procedures recommended in IEC 60060-1, (2) the other is the method by taking the voltage at the instant of chopping against the time to breakdown. As a result, the V-t characteristics of $SF_6-N_2$ mixtures in nonuniform electric field were significantly affected by the polarity and wave shape of the applied voltages. The positive breakdown voltages resulted in lower breakdown voltages in the time ranges considered, and the V-t curves for the negative oscillatory impulse voltage were extended over the longer time range. For the lightning impulse voltages, the V-t curves obtained by IEC Pub. 60060-1 were nearly same with the V-t curves obtained by the voltage at the instant of chopping against the time to breakdown. It is clear that the actual breakdown voltages were much lower than the maximum voltages appearing at or prior to breakdown because of the displacement current produced as a result of the dV/dt during the oscillatory transient voltage app1ication. The scattering of the negative actual breakdown voltages was much larger than that of the positive.

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일반쌀 및 다수확 쌀의 수화속도 (Kinetic Studies on Hydration of Traditional and High-Yielding Rice Varieties)

  • 이순옥;김성곤;이상규
    • Applied Biological Chemistry
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    • 제26권1호
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    • pp.1-7
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    • 1983
  • 일반 품종(아끼바레와 밀양 15) 및 다수확품종(밀양 30, 수원 287, 수원 294와 이리 342)의 벼를 무게비로 8% 도정하고, 쌀을 온도 $4{\sim}32^{\circ}C$에서 $5{\sim}50$분간 침지시키면서 수화속도를 비교하였다. 침지시간 50분후의 쌀의 평형 수분함량은 아끼바레와 밀양 15가 30%내외, 수원 287과 밀양 30이 29%내외이었고, 수원 294와 이리 342는 다소 낮은 값을 보였다. 물의 확산계수는 아끼바레는 밀양 14와, 밀양 30은 수원 287과, 수원 294는 이리 342와 비슷한 값을 보였다. 확산계수는 밀양 30과 수원 287이 가장 컸으며, 수원 294와 이리 342가 가장 작았다.

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Single-Stage High-Power-Factor Electronic Ballast with a Symmetrical Class-DE Resonant Rectifier

  • Ekkaravarodome, Chainarin;Jirasereeamornkul, Kamon
    • Journal of Power Electronics
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    • 제12권3호
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    • pp.429-438
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    • 2012
  • This paper presents the use of a novel, single-stage high-power-factor electronic ballast with a symmetrical class-DE low-$d{\upsilon}$/$dt$ resonant rectifier as a power-factor corrector for fluorescent lamps. The power-factor correction is achieved by using a bridge rectifier to utilize the function of a symmetrical class-DE resonant rectifier. By employing this topology, the peak and ripple values of the input current are reduced, allowing for a reduced filter inductor volume of the EMI filter. Since the conduction angle of the bridge rectifier diode current was increased, a low-line current harmonic and a power factor near unity can be obtained. A prototype ballast, operating at an 84-kHz fixed frequency and a 220-$V_{rms}$, 50-Hz line input voltage, was utilized to drive a T8-36W fluorescent lamp. Experimental results are presented which verify the theoretical analysis.

Comprehension of the Response Time in a Microbial BOD Sensor(II)

  • Sohn, Moo-Jeong;Hong, Dae-Il
    • Bulletin of the Korean Chemical Society
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    • 제14권6호
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    • pp.666-668
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    • 1993
  • A microbial BOD sensor using immobilized Hansenula anomala was prepared for the estimation of BOD. The sensor voltage was increased with time and increasing concentration of GGA when it was inserted in a sample solution. A linear relationship was obtained with a correlation coefficient, 0.998 between the concentration of standard GGA solutions and dV/dt by using the initial change of voltage, in which the response time was 20 min. It could be concluded that the oxidation of GGA conformed to a first-order kinetics. Therefore, the good linearities were also observed at various times. This sensor showed the best linearity at 30 min.

Installation of Induced Current Measurement Systems in Substations and Analysis of GIC Data during Geomagnetic Storms

  • Choi, Kyu-Cheol;Park, Mi-Young;Ryu, Youngsoo;Hong, Youngsu;Yi, Jong-Hyuk;Park, Sung-Won;Kim, Jae-Hun
    • Journal of Astronomy and Space Sciences
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    • 제32권4호
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    • pp.427-434
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    • 2015
  • Coronal Mass Ejections (CME), which originate from active regions of the Sun's surface, e.g., sunspots, result in geomagnetic storms on Earth. The variation of the Earth's geomagnetic field during such storms induces surface currents that could cause breakdowns in electricity power grids. Hence, it is essential to both monitor Geomagnetically Induced Currents (GICs) in real time and analyze previous GIC data. In 2012, in order to monitor the variation of GICs, the Korean Space Weather Center (KSWC) installed an induced current measurement system at SINGAPYEONG Substation, which is equipped with 765 kV extra-high-voltage transformers. Furthermore, in 2014, two induced current measurement systems were installed on the 345 kV high-voltage transformers at the MIGEUM and SINPOCHEON substations. This paper reports the installation process of the induced current measurement systems at these three substations. Furthermore, it presents the results of both an analysis performed using GIC data measured at the SINGAPYEONG Substation during periods of geomagnetic storms from July 2013 through April 2015 and the comparison between the obtained GIC data and magnetic field variation (dH/dt) data measured at the Icheon geomagnetic observatory.

Ag Pastes의 분산 특성 및 스크린 인쇄된 OTFTs용 전극 물성 (Dispersion Characteristics of Ag Pastes and Properties of Screen-printed Source-drain Electrodes for OTFTs)

  • 이미영;남수용
    • 한국전기전자재료학회논문지
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    • 제21권9호
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    • pp.835-843
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    • 2008
  • We have fabricated the source-drain electrodes for OTFTs by screen printing method and manufactured Ag pastes as conductive paste. To obtain excellent conductivity and screen-printability of Ag pastes, the dispersion characteristics of Ag pastes prepared from two types of acryl resins with different molecular structures and Ag powder treated with caprylic acid, triethanol amine and dodecane thiol as surfactant respectively were investigated. The Ag pastes containing Ag powder treated with dodecane thiol having thiol as anchor group or AA4123 with carboxyl group(COOH) of hydrophilic group as binder resin exhibited excellent dispersity. But, Ag pastes(CA-41, TA-41, DT-41) prepared from AA4123 fabricated the insulating layer since the strong interaction between surface of Ag powder and carboxyl group(COOH) of AA4123 interfered with the formation of conduction path among Ag powders. The viscosity behavior of Ag pastes exhibited shear-thinning flow in the high shear rate range and the pastes with bad dispersion characteristic demonstrated higher shear-thinning index than those with good dispersity due to the weak flocculated network structure. The output curve of OTFT device with a channel length of 107 ${\mu}m$ using screen-printed S-D electrodes from DT-30 showed good saturation behavior and no significant contact resistance. And this device exhibited a saturation mobility of $4.0{\times}10^{-3}$ $cm^2/Vs$, on/off current ratio of about $10^5$ and a threshold voltage of about 0.7 V.

Gyroklystron Tube 구동을 위한 고전압 펄스 전원장치의 설계 및 개발 (Development of High Voltage Pulse Power Supply for Gyroklystron Tube)

  • 박재안;윤영대
    • 대한전기학회:학술대회논문집
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    • 대한전기학회 2000년도 학술대회 논문집 전문대학교육위원
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    • pp.71-73
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    • 2000
  • 최근 고 에너지 저장 및 발생장치의 개발은 군사용에서 산업용으로 응용되면서 각종 첨단 설비가 개발되고 있다. 본 논문에서는 전자빔 발생기로 쓰이는 Gyroklystron용 대전력, 고전압, 전류 펄스 전원장치로 입력부, 특고압 발생부, 고압 정류부 및 IGBT 펄스 스위치 구성하고 그 설계 및 개발 자료에 대하여 기술하였다. 대전력 고전압 전류펄스 전원장치를 위한 각 구성 부분의 제어 및 설계 특징은 다음과 같다. 입력부인 IGBT Inverter는 펄스 전원장치의 제어를 위하여 출력 고전압을 Feedbark System에 의해 펄스 설정 전압을 유지하도록 제어하며, 또한 펄스 출력중에 직류 고전압부의 전압강하, 즉 펄스 진압의 Drop이 커지는 것을 방지하기 위하여 Fast Dynamics를 갖도록 Feedback System을 구성하였다. 단상 특고압 승압용 변압기 3대를 직렬접속한 특고압 발생부는 PWM 제어된 전압을 입력받아 특고압으로 승압시키며 고압 펄스성 전압과 매우 높은 dV/dt 전압이 인가되므로 Stray Capacitance가 최소가 되어야 하며 절연파괴로부터 보호될 수 있어야 한다. 고압 정류부는 Inverter와 특고압 변압기에 의하여 전원이 공급되므로 교류전압의 교번 순간에 매우 높은 전압변동률을 가지는 Fast Recovery High Voltage Rectifier로 설계 제작되어졌다. 펄스 스위치인 IGBT 스위치는 Gate Driver에 의해 구동되어 지며 주어진 펄스 사양을 만족시키게 된다. 특히 소자의 전압특성을 고려하여 120KV의 전압 값을 갖도록 설계, 제작하였다.

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Electron Beam Gun 구동을 위한 고전압 펄스 전원장치 개발 (Development of High Voltage Pulse Power Supply for Electron Beam Gun)

  • 박재안;이용운;박성태;이경수;정병웅
    • 대한전기학회:학술대회논문집
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    • 대한전기학회 2000년도 하계학술대회 논문집 B
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    • pp.1309-1311
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    • 2000
  • 본 논문에서는 입력부, 특고압 발생부 및 고압 정류부, IGBT Pulse Switch로 구성된 Gyro-klystron용 대전력, 고전압, 전류 펄스 전원장치의 설계 및 개발에 대하여 기술하였다. 대전력, 고전압, 전류 펄스 전원장치를 위한 각 구성부분의 제어 및 설계 특징은 다음과 같다. 입력부인 IGBT Inverter는 펄스 전원장치의 전압 제어를 위하여 출력 고전압을 Feedback System 제어에 의해 Pulse 설정 전압을 갖도록 제어하며, 또한 Pulse 출력중에 직류 고전압부의 전압강하, 즉 Pulse 전압의 Drop이 커지는 것을 방지하기 위하여 Fast Dynamics를 갖도록 Feedback System을 구성하였다. 3대의 단상 특고압 승압변압기가 직렬로 구성된 특고압 발생부는 PWM된 전압을 입력받아 특고압으로 승압시킨다. 특고압 변압기는 고압 Pulse성 전압과 매우 높은 dV/dt 전압이 인가되므로 Stray Capacitance가 최소가 되어야 하며 절연파괴로부터 보호될 수 있어야 한다. 고압 정류부는 Inverter와 특고압변압기에 의하여 전원이 공급되므로 교류전압의 교번순간에 매우 높은 전압 변동률을 가지는 Fast Recovery High Voltage Rectifier로 설계, 제작되어졌다. Pulse Switch인 IGBT Switch는 Gate Driver에 의해 구동되어 진다. 주어진 Pulse 사양을 만족시키며 특히 소자의 전압 특성을 고려하여 120KV의 전압값을 갖도록 설계, 제작하였다. 본 논문에서는 고전압 펄스 전원장치 각 부분의 설계에 대하여 기본적인 사항들을 제시하며, 실험결과를 통하여 제안된 방식의 우수한 특성을 입증한다.

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Particle-in-cell simulation feasibility test for analysis of non-collective Thomson scattering as a diagnostic method in ITER

  • Zamenjani, F. Moradi;Asgarian, M. Ali;Mostajaboddavati, M.;Rasouli, C.
    • Nuclear Engineering and Technology
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    • 제52권3호
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    • pp.568-574
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    • 2020
  • The feasibility of the particle-in-cell (PIC) method is assessed to simulate the non-collective phenomena like non-collective Thomson scattering (TS). The non-collective TS in the laser-plasma interaction, which is related to the single-particle behavior, is simulated through a 2D relativistic PIC code (XOOPIC). For this simulation, a non-collective TS is emitted from a 50-50 DT plasma with electron density and temperature of ne = 3.00 × 1013 cm-3 and Te = 1000 eV, typical for the edge plasma at ITER measured by ETS system, respectively. The wavelength, intensity, and FWHM of the laser applied in the ETS system are λi,0 = 1.064 × 10-4 cm, Ii = 2.24 × 1017 erg=s·㎠, and 12.00 ns, respectively. The electron density and temperature predicted by the PIC simulation, obtained from the TS scattered wave, are ne,TS = 2.91 × 1013 cm-3 and Te,TS = 1089 eV, respectively, which are in accordance with the input values of the simulated plasma. The obtained results indicate that the ambiguities rising due to the contradiction between the PIC statistical collective mechanism caused by the super-particle concept and the non-collective nature of TS are resolved. The ability and validity to use PIC method to study the non-collective regimes are verified.

THREE-SITE PHOTOMETRIC MONITORING OF THE δ SCT-TYPE PULSATING STAR V1162 ORIONIS : PERIOD CHANGE AND ITS IMPLICATIONS FOR PRE-MAIN SEQUENCE EVOLUTION

  • KIM, SEUNG-LEE;CHA, SANG-MOK;LIM, BEOMDU;LEE, JAE WOO;LEE, CHUNG-UK;LEE, YONGSEOK;KIM, DONG-JIN;LEE, DONG-JOO;KOO, JAE-RIM;HONG, KYEONGSOO;RYU, YOON-HYUN;PARK, BYEONG-GON
    • 천문학회지
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    • 제49권5호
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    • pp.199-208
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    • 2016
  • We present photometric results of the δ Sct star V1162 Ori, which is extensively monitored for a total of 49 nights from mid-December 2014 to early-March 2015. The observations are made with three KMTNet (Korea Microlensing Telescope Network) 1.6 m telescopes installed in Chile, South Africa, and Australia. Multiple frequency analysis is applied to the data and resulted in clear detection of seven frequencies without an alias problem: five known frequencies and two new ones with small amplitudes of 1.2-1.7 mmag. The amplitudes of all but one frequency are significantly different from previous results, confirming the existence of long-term amplitude changes. We examine the variations in pulsation timings of V1162 Ori for about 30 years by using the times of maximum light obtained from our data and collected from the literatures. The O − C (Observed minus Calculated) timing diagram shows a combination of a downward parabolic variation with a period decreasing rate of (1/P)dP/dt = −4.22 × 10−6 year−1 and a cyclic change with a period of about 2780 days. The most probable explanation for this cyclic variation is the light-travel-time effect caused by an unknown binary companion, which has a minimum mass of 0.69 M. V1162 Ori is the first δ Sct-type pulsating star of which the observed fast period decrease can be interpreted as an evolutionary effect of a pre-main sequence star, considering its membership of the Orion OB 1c association.