석탄회를 이용한 석탄광산 폐기물의 안정화 효율성 평가

오세진(Se-Jin Oh),김성철(Sung-Chul Kim),고주인(Ju-In Ko),이진수(Jin-Soo Lee),양재의(Jae E. Yang) 한국토양비료학회 2011 한국토양비료학회지 Vol.44 No.6

본 연구는 다량의 중금속을 함유하는 폐석탄 광산에 적치된 폐석으로부터 발생하는 침출수의 안정화를 위해 석탄회를 안정화제로서의 적용성을 평가하는데 목적이 있다. 석탄폐석에 석탄회를 적용하여 컬럼시험을 수행한 결과는 다음과 같다. 1) 석탄회의 pH는 비산재와 바닥재가 각각 11.1, 9.7의 강알칼리성을 갖는 것으로 나타나 강산성 조건의 폐석 (pH 3.5)를 교정하였으며 유기물을 비롯하여 식물생장에 필요한 영양소인 인산, 칼슘 등을 함유하는 것으로 나타나 폐석과 혼합할 경우 비옥도가 개선될 수 있을 것으로 판단된다. 2) 폐석만을 충진한 컬럼에서 발생하는 침출수의 pH는 3.5~4.0의 수준을 시험기간 동안 지속적으로 유지하는 것으로 나타나지만, 석탄회의 처리량에 따라 40% (pH 5.0~6.0) 〉 20% (pH 4.5)로 나타나고, 동일 처리량 (40%)의 처리방법에 따른 효율성은 완전혼합 (pH& & 5.0~6.0) 방법이 층위처리 (pH 4.0~4.5)에 비해 pH 상승효과가 높은 것으로 조사되었다. 3) 침출수의 Ca과 Mg의 함량은 4 pore volume까지 빠르게 용탈되다 그 이후부터 안정화 되었으며 석탄회에서 용탈된 Ca과 Mg의 영향으로 폐석에 함유되었던 Cu, Pb, As, 및 Al 등이 탄산이온 (CO₃<SUP>2-</SUP>) 또는 수산화이온 (OH-)과 불용성 화합물을 형성하여 안정화 되는 것으로 사료된다. 4) 철의 용존함유량에 대한 분석결과 석탄회 처리구의 용존량이 석탄회를 40% 층위처리한 처리구를 제외하고 대조구에 비해 약 8-74% 정도 감소하는 것으로 조사 되었다. 5) 석탄회를 이용한 폐석의 중화 및 철의 용존량 감소 효율성을 평가한 결과 폐석의 중화 효율성은 석탄회를 40% 완전혼합한 경우 가장 높았으며 철의 용존량 감소 효율성은 석탄회를 20% 완전혼합한 경우가 가장 좋은 것으로 조사되었다. 따라서 석탄회를 이용하여 현장에서 폐석을 처리할 경우 약 20-40%의 석탄회를 처리해야 높은 효율성을 얻을 수 있을것으로 사료된다. In this study, coal combustion ash (CCA) was evaluated for its stabilization effect on acidic mine waste with column experiment. Total of six treatments were installed depending on mixing ratio between coal wastes and CCA (0, 20, 40%) and mixing method (completely mixing and layered). Artificial acidic rain (pH 5.6) was used for feeding solution with flow rate of 0.05 mL min<SUP>-1</SUP>. Result showed that higher pH of leachate was observed as more CCA was mixed. The highest pH in leachate was measured when 40% of CCA was mixed with coal waste (pH of 5.8). Also, complete mixing with CCA and coal waste was more effective to increase the pH of leachate than layered treatment. Regarding the reduction of soluble Fe amount, the highest efficiency (78%) was observed when 20% of coal ash was completely mixed with mine waste. Based on those result, optimum mixing ratio of coal ash with mine waste can be ranged 20-40% depending on environmental circumstances in the field.

다중표적 환경에서 추적시스템을 위한 연동 소프트웨어 모듈 연구

오세진,Oh, Se-Jin 한국군사과학기술학회 2011 한국군사과학기술학회지 Vol.14 No.4

In this paper, you can see the structure of data slaving software module that is in use on flight test and result of the test with the slaving. The data slaving software module has many functions, data slaving for various instrumentation systems(instrumentation radars, telemetry systems for missile, aircraft and so on), setting some slaving group for multi-target, communicating with the instrumentation systems in a far away site and sending a specific value as slaving data. This fits the requests for flight test that is being performed and improves performance of the instrumentation systems.

관측 데이터의 고속기록을 위한 대용량 저장시스템

오세진,노덕규,김광동,송민규,제도흥,위석오,김태성,OH SE-JIN,ROH DUK-GYOO,KIM KWANG-DONG,SONG MIN-GYU,JE DO-HEUNG,WI SEOG-OH,KIM TAE-SUNG,WHITNEY ALAN R. 한국천문학회 2004 天文學論叢 Vol.19 No.1

In this paper, we introduce the development of the large storage system in order to record the observed space radio signal in the Korean VLBI Network(KVN) with high-speed. The KVN is the Very Long Baseline Interferometery(VLBI) to observe the birth of star, the structure of space by constructing radio telescope with diameter 21m at the Seoul, Ulsan, Jeju from 2001 to 2007 years. To do this, Korea Astronomy Observatory joined the international consortium for developing the high-speed large storage system(Mark 5), which is developed by MIT Haystack observatory. The Mark 5 system based on hard disk has to record up to 1 Gbps the observed space radio signal. The main features of Mark 5 system are as follows; First it is able to directly record the input data to the hard disk without PC1(Peripheral Component Interconnect) internal bus, and the second, it has two hard disk banks, which are able to hot-swap ATA/IDE type very cheap up to 1 Gbps recording and playback. The third is that it follows the international VLBI standard interface hardware(VSI-H). Therefore it can be connect directly the VSI-H type system at the input/output. Finally it also supports e- VLBI(Electronic-VLBI) through the standard Gigabits Ethernet connection.

KVN의 광대역 관측 시험 및 결과고찰

오세진,오야마 토모아키,염재환,니시카와다카시,노덕규,김승래,이의겸,제도흥,변도영,이성모,정현수,Oh, Se-Jin,Oyama, Tomoaki,Yeom, Jae-Hwan,Nishikawa, Takashi,Roh, Duk-Gyoo,Kim, Seung-Rae,Lee, Eui-Gyeom,Je, Do-Heung,Byun, Do-Young,Lee, Seong-Mo,C 한국융합신호처리학회 2016 융합신호처리학회 논문지 (JISPS) Vol.17 No.2

본 논문에서는 한국우주전파관측망의 성능 확장을 위해 광대역 관측시스템의 시험 및 결과에 대해 소개한다. KVN은 1024Mbps 속도로 VLBI 관측을 수행하는데, 4주파수 동시관측을 위한 8192Mbps 관측은 정규 운영을 위해 시험하고 있다. 세계 여러 VLBI 관측국에서는 높은 정밀도와 고분해능의 천체를 관측하기 위해 광대역 관측시스템을 독자적으로 개발하거나 여러 나라와 협력하고 있다. KVN은 K/Q//W/D 밴드의 RF 신호를 주파수 변환을 하지 않고 한 주파수 대역에 대해 최대 2048MHz 대역폭을 직접 샘플링하는 OCTAD 고속샘플러를 도입할 계획이다. 따라서 KVN의 성능확장을 위한 사전연구로서 일본국립천문대와의 협력을 통하여 OCTAD 고속샘플러와 데이터 기록을 위한 OCTADISK2 고속기록기를 현장에 설치한 후, 광대역 관측시험을 통하여 성능을 확인하고 그 결과를 본 논문에서 고찰하고자 한다. In this paper, we introduce the results of the testing and observation systems for performance wideband expansion in the Korean VLBI Network(KVN). The KVN performs VLBI observations to 1024 Mbps data rate, and 8192 Mbps observing for four simultaneous observation is now evaluating for normal operation. The VLBI stations in several world countries developed their own wideband observing systems to observe the celestial objects with high precision and high resolution or are working with several countries. The KVN is planning to introduce a high-speed sampler, OCTAD, for sampling directly up to 2048 MHz bandwidth for RF signal of K/Q/W/D band in the frequency band without conversion. Therefore, as a preliminary study for the performance scalability of the KVN then through the close cooperation with National Astronomical Observatory of Japan (NAOJ), the OCTAD high-speed sampler and OCTADISK2 high-speed recorder were installed in the KVN Yonsei station, and verify the performance through a wideband.

VLBI의 기준 주파수와 시각 동기 시스템

오세진,정현수,노덕규,김광동,OH SE-JIN,CHUNG HYUN-SOO,ROH DUK-GYOO,KIM KWANG-DONG 한국천문학회 2004 天文學論叢 Vol.19 No.1

In this paper, we describe a principle of the atomic frequency standard and clock system in VLBI(Very Long Baseline Interferometry). The hydrogen maser is a usual VLBI standard. During VLBI observations, signals emitted by distant sources of radio frequency energy(quasars) are received and recorded at several antennas. At each antenna(VLBI station), a very stable frequency standard(hydrogen maser) provides a reference signal which enables time-tagging to the quasar signals as they are being recorded on magnetic tapes or hard-disk modules. For each VLBl experiment, correlation of the time-tagged recorded information between the participating antennas is used to yield the arrival time differences of any specific quasar radio wave between the antennas. These time differences are used to calculate the relative antennas to each other. In this paper, we also introduce the KVN(Korean VLBI Network) atomic frequency standard and clock system.

한국우주전파관측망(KVN)을 위한 시각 시스템 구축과 성능측정

오세진,제도흥,이창훈,노덕규,정현수,변도영,김광동,김효령,정구영,안우진,황정욱,Oh, Se-Jin,Je, Do-Heung,Lee, Chang-Hoon,Roh, Duk-Gyoo,Chung, Hyun-Soo,Byun, Do-Young,Kim, Kwang-Dong,Kim, Hyo-Ryung,Jung, Gu-Young,Ahn, Woo-Jin,Hwang, Jeong 한국천문학회 2007 天文學論叢 Vol.22 No.4

In this paper, we describe the proposed KVN (Korean VLBI Network) clock system in order to make the observation of the VLBI effectively. In general, the GPS system is widely used for the time information in the single dish observation. In the case of VLBI observation, a very high precise frequency standard is needed to perform the observation in accordance with the observation frequency using the radio telescope with over 100km distance. The objective of the high precise clock system is to insert the time-tagging information to the observed data and to synchronize it with the same clock in overall equipments which used in station. The AHM (Active Hydrogen Maser) and clock system are basically used as a frequency standard equipments at VLBI station. This system is also adopted in KVN. The proposed KVN clock system at each station consists of the AHM, GPS time comparator, standard clock system, time distributor, and frequency standard distributor. The basic experiments were performed to check the AHM system specification and to verify the effectiveness of implemented KVN clock system. In this paper, we briefly introduce the KVN clock system configuration and experimental results.

PC를 이용한 소규모 기가비트 VLBI 관측시스템

오세진,노덕규,김광동,정현수,제도흥,위석오,한석태,김현구,Oh, Se-Jin,Roh, Duk-Gyoo,Kim, Kwang-Dong,Chung, Hyun-Soo,Je, Do-Heung,Wi, Seog-Oh,Han, Seog-Tae,Kim, Hyun-Goo 한국천문학회 2005 天文學論叢 Vol.20 No.1

In this paper, we propose a small-scale Gigabit VLBI observing system for the Korean VLBI Network (KVN) under construction. The system consists of high-speed sampler, IP-VLBI board, PC-VSI board, and software correlator. Radio signal received by receiver is sampled by high-speed sample. at 1 Gsps (Gigabit sample per second) rate with 2 bits quantization. The digitized signal is recorded in PC and the software correlator does the cross correlation. IP-VLBI board will be used for the geodesy VLBI observation, while PC-VSI board is for the astronomical VLBI observation. The PC-VSI board adopts the VSI-H (VLBI Standard Interface Hardware). The proposed system is based on commercial PCs and therefore can be built inexpensively.

VLBI상관서브시스템의 검증을 위한 소프트웨어 시뮬레이터의 개발 및 성능시험

오세진,노덕규,염재환,정현수,이창훈,김효령,김광동,강용우,박선엽,Oh, Se-Jin,Roh, Duk-Gyoo,Yeom, Jae-Hwan,Chung, Hyun-Soo,Lee, Chang-Hoon,Kim, Hyo-Ryoung,Kim, Kwang-Dong,Kang, Yong-Woo,Park, Sun-Yeop 한국천문학회 2008 天文學論叢 Vol.23 No.2

A software simulator is developed for verifying the VLBI Correlation Subsystem (VCS) trial product hardware. This software simulator includes the delay tracking, fringe rotation, bit-jump, FFT analysis, re-quantization, and auto/cross-correlation functions so as to confirm the function of the VCS trial product hardware. To verify the effectiveness of the developed software simulator, we carried out experiments using the simulation data which is a mixed signal with white noise and tone signal generated by software. We confirmed that the performance of this software simulator is similar as that of the hardware system. In case of spectral analysis and re-quantization experiment, a serious problem of the VCS hardware, which is not enough for expressing the data stream of FFT results specified in VCS hardware specification, was found by this software simulator. Through the experiments, the performance of software simulator was verified to be efficient. In future, we will improve and modify the function of software simulator to be used as a software correlator of Korea-Japan Joint VLBI Correlator (KJJVC).

대전 상관기의 전처리를 위한 광역 프린지 탐색 소프트웨어 개발 및 시험

오세진,노덕규,윤영주,염재환,오충식,쿠라야마 토모하루,정동규,정진승,Oh, Se-Jin,Roh, Duk-Gyoo,Yun, Young-Joo,Yeom, Jae-Hwan,Oh, Chung-Sik,Kurayama, Tomoharu,Chung, Dong-Kyu,Jung, Jin-Seung 한국융합신호처리학회 2014 융합신호처리학회 논문지 (JISPS) Vol.15 No.4

본 논문에서는 대전상관기의 전처리를 위한 광역 프린지 탐색 소프트웨어 개발에 대해 기술한다. VLBI 관측의 경우 전파망원경에 의해 천체를 잘 관측하였는지 확인하기 위해 관측자는 관측일정에서 잘 알려져 있는 전파세기가 강하고 밝은 천체(포인터 소스, 참조천체)를 목적천체와 함께 관측을 수행한다. 상관기는 참조천체를 대상으로 상관 프린지가 잘 검출되는지 확인하는 전처리를 수행한다. 본 논문에서는 특정 관측국을 기준으로 각 관측국 사이의 정확한 지연시각을 계산하는 GFS 소프트웨어를 개발하였는데, 이 소프트웨어는 상관 전처리를 통하여 각 관측국에 위치한 수소원자시계와 GPS 시각 사이의 시각오차 정보 및 참조천체의 지연모델(상관모델)을 이용하여 정확한 지연시각을 계산한다. 개발한 소프트웨어의 성능을 확인하기 위한 상관 전처리 시험을 KaVA 관측망으로 관측한 참조천체와 목적천체에 대해 수행하였다. 시험결과는 GFS 소프트웨어로 찾은 지연시각 오차를 보정한 결과와 그렇지 않은 것의 비교에 따라 매우 좋은 성능을 보여 효과적임을 나타내었다. This paper introduces the development of global fringe search (GFS) software for preprocessing of Daejeon Correlator. In case of the VLBI observation, a observer conducts the observation for the reference sources with strong and point-like radio stars on schedule in order to confirm the well-observedness of the radio source by the radio telescope. The correlator performs the correlation for the reference sources to detect the fringe completely. We developed the GFS software by calculating the precise delay time between each observatory based on specific observatory. Then, this software calculates the precise delay time by using the delay model (correlator model) of reference source and information of time offset between the Hydrogen Maser frequency standard and GPS (Global Positioning System) clock located in each observatory through the correlation preprocessing. In order to confirm the performance of the developed software, experiments were carried out for the reference sources and target sources observed by the KaVA (KVN and VERA Array). Experimental results show that the GFS software has effectively good performance by finding the precise delay time offset according to the comparison between the compensated delay time offset and one without compensation.

대전상관기에서 복층패턴 문제의 해결에 관한 연구

오세진,노덕규,염재환,정동규,오충식,황주연,Oh, Se-Jin,Roh, Duk-Gyoo,Yeom, Jae-Hwan,Chung, Dong-Kyu,Oh, Chung-Sik,Hwang, Ju-Yeon 한국융합신호처리학회 2015 융합신호처리학회 논문지 (JISPS) Vol.16 No.4

본 논문에서는 한일상관센터에서 운영하고 있는 대전상관기의 복층패턴에 대한 원인과 문제 해결에 대해 기술한다. 대전상관기의 상관결과에서 입력신호의 전력파워가 잡음에 묻힐 정도로 작은 경우에는 잘 보이지 않지만, 전력파워가 큰 경우 입력신호에 특정한 패턴을 가진 신호가 출현하는 문제가 보고되었다. 이는 관측데이터의 상관결과와 소프트웨어 상관기와 비교하여 AIPS 소프트웨어에서 분석할 때 관측결과의 천체신호 진폭이득에는 3% 정도의 영향을 미치고 있음이 확인되었다. 따라서 복층패턴의 문제를 해결하기 위해 주기적으로 발견되는 복층패턴의 원인으로 상관기의 데이터 입력과 직렬화를 담당하는 모듈에서 메모리 관리 영역에 문제가 있음을 발견하였다. 즉, 직렬화 모듈에서 데이터를 직렬화할 때 할당된 각 메모리 영역의 데이터가 반복적으로 읽혀져 직렬화되면서 중복된 데이터가 마지막으로 할당된 메모리의 데이터와 중첩이 되면서 발생하는 것이다. 따라서 직렬화 모듈의 메모리 관련 영역의 FPGA 프로그램을 수정하여 문제를 해결하여, 정상적인 상관결과가 출력되는 것을 확인하였다. This paper describes the reason and the problem solving for the double-layer pattern of a Daejeon correlator operated in Korea-Japan Correlation Center. When the electric power of an input signal in the correlator is charged small enough to be buried in the noise, it is hard to see a signal with a specific pattern in the input signal, but when the electric power is large, a specific one is reported to be seen. By comparing data from observation with one from software correlator, it was confirmed from the analysis using the AIPS software that the amplitude gain of a source signal was affected about 3%. Therefore, in order to solve the problem of double-layer patterns, we found that a problem in the memory management module responsible for both the data input and the data serialization of the correlator is a cause for the double-layer pattern detected periodically. In other words, while data is serialized and read repeatedly in the memory area assigned to serialize the data from the serialization module, redundant last data is generated and an overlap for the memory allocation is occurred. Therefore, by modifying the program of the FPGA memory sections on serialization module to correct the problem, we confirmed that double-layer pattern is disappeared and correlation results are normally acquired.