• 제목/요약/키워드: Radiation spectrum

검색결과 504건 처리시간 0.023초

기관지 선종의 외과적 치료[17례 보고] (Surgical Treatment of Bronchial Adenoma - Reports of 17 Cases -)

  • 문석환
    • Journal of Chest Surgery
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    • 제25권3호
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    • pp.247-257
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    • 1992
  • Bronchial adenoma, firstly described by Muller[1882] had been reported on the subject stressed their benign nature prior to 1940`s, but these tumors including carcinoid tumor, mucoepidermoid carcinoma, adenoid cystic carcinoma, pleomorphic adenoma are now known to possess the various degree of malignant natures from benign course, low grade malignant potential to distant lymphatic or hematogenous metastasis or combination. Although histologically diffeerent, four varieties except carcinoid tumor which is a spectrum of neu-roendocrine tumor originating Kulchitsky cell of the bronchial epithelium and form the part of the APUD tumor spectrum, are morphologically and in many respects clinically similar to the corresponding tumor of the salivary gland is a specific varient of adenocarcinoma that occurs most commonly in the major and minor salivary gland and less frequently tra-cheobronchial tree, esophagus etc. To better understand the clinical characteristics and assess more precisely the malignat nature of bronchial adenoma, we studied 17 cases of bronchial adenoma, which had been experienced at the Department of Thoracic and Cardiovascular surgery of Catholic University Medical College from April 1977 to september 1991. Seventeen cases of bronchial adenoma consist of 2 carcinoid tumors, 6 adenoid cystic carcinomas, 8 mucoepidermoid carcinomas and one pleomorphic adenoma. There is a slight predominace of male patients[10/17] and the age of pt studied varied with a higher incidence occurring between the ages of 40 years and 60 years[mean age, 46.5 years]; the youngest being 15 years and oldest 69 years. Their leading complaints were hemoptysis[4], exertional dyspnea[8], fever & chilness [4], and symptoms mimicking the bronchial asthma[4]. Diagnosis was aided by the radiologic studies such as chest X-ray, polytomography, CT scan, brochography and bronchoscopy. The preferred locations of fumor were in the trachea[4], main stem bronchus[3], bronchus intermedius[3], bronchus of RUL[2], LUL[1], RLL[1], LLL[3] with no peripheral location. Modalities of treatments were single or combination of surgical resection, radiation therapy, chemotherapy. Complete resections were permitted in 12 cases with late recurrences of 4 cases ranging from 6 months to 10 years: pneumonectomy[4], lobectomy[4], bil-obectomy[2], sleeve resection[2]. Gross findings of resected specimens in 14 cases showed that 4 cases were polyp-like pedunculated mass[entirely intraluminal mass] with intact mucosa, 8 cases were broad-bas-ed sessile mass[predominatly intraluminal] and the main portions were located below the mucosa similar to tip of iceburg[predominantly extraluminal] in 2 cases. Follow-up information was availble in all 17 cases ; eight were alive without evidence of disese ranging from 1 month to 13 years. But seven cases died of the causes related to tumor[6 cases within 12 months, one case 10 years after pneumonectomy]. We concluded that 8 cases[47%] of 17 cases were metastasizing bronchial adenoma and precise survival rate cannot be answered by the scanty materials available for study.

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GEANT4 Medical Linac2 예제를 이용한 6 MV 선형가속기 광자선속의 기초특성과 연구방법 (Study on the 6 MV Photon Beam Characteristics and Analysis Method from Medical Linear Accelerators Using Geant4 Medical Linac2 Example)

  • 김병용;김형동;김성진;오세안;강정구;김성규
    • 한국의학물리학회지:의학물리
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    • 제22권2호
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    • pp.79-84
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    • 2011
  • 본 연구에서는 GEANT4 toolkit을 이용하여 의료용 선형가속기에 대한 몬테칼로(Monte Carlo) 전산모사를 하였다. Medical Linac2 예제를 수정해서 사용하였다. 에너지스펙트럼, 최빈에너지, 평균에너지를 EGS4 결과와 비교 하였고 선속의 중심에서부터 반경에 따른 단위면적당 광자수, 단위면적당 에너지, 평균에너지를 분석하였다. 그 결과 EGS4 결과와 큰 차이를 보이지 않기 때문에 Medical Linac2 예제의 선속특성에 관한 전산모사에 큰 문제점은 없는 것으로 판단된다. 같은 헤드구조에서도 Physics List의 모델에 따라서는 결과에 차이가 발생하므로 연구 환경에 알맞은 Physics List 모델을 선택하는 것이 중요하다고 판단된다. 본 연구는 처음 몬테칼로 전산모사를 접하는 사용자가 선속특성에 대한 전산모사를 수행하고 6 MV 광자선속의 특성을 분석하는 과정에 많은 도움이 될 것으로 사료된다.

Green Light-Emitting Phosphor, Ba2xCaMgSi2O8:Eux

  • Kim, Jeong-Seog;Piao, Ji-Zhe;Choi, Jin-Ho;Cheon, Chae-Il;Park, Joo-Suk
    • 한국세라믹학회지
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    • 제42권3호
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    • pp.145-149
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    • 2005
  • [ $Eu^{2+}$ ]-activated barium magnesium silicate phosphor, $(Ba,Ca)_{3}MgSi_{2}O_{8}:Eu_{x}$, has been known to emit blue-green light. In this study we report the manufacturing processes for producing either pure green or pure blue light-emitting phosphor from the same composition of $Ba_{2-x}Ca_{2}CaMgSi_{2}O_{8}:Eu_{x}$ (0 < x < 1) by controlling heat treatment conditions. Green light emitting phosphor of $Ba_{1.9}CaMgSi_{2}O_{8}:Eu_{0.1}$ can be produced under the sample preparation condition of highly reducing atmosphere of $23\%\;H_2/77\%\;N_2$, while blue or blue-green light emitting phosphor under reducing atmosphere of $5\~20\%\;H_2\;/\;95\~80\%$ N_2. The green light-emitting phosphors are prepared in two steps: firing at $800\~1000^{\circ}C$ for $2\~5$ h in air then at $1100\~1350^{\circ}C$ for 2-5 h under reducing atmo­sphere $23\%$ $H_2/77\%\;N_2$. The excitation spectrum of the green light-emitting phosphor shows a broadband of $300\~410$ nm. The emission spectrum has a maximum intensity at the wavelength of about 501 nm. The CIE value of green light emission is (0.162, 0.528). The pure blue light-emitting phosphors can be produced using the $Ba{2_x}CaMgSi_{2}O_{8}:Eu_{x}$ by introducing additional firing step at $1150\~1300^{\circ}C$ in air before the final reducing treatment. The XRD analysis shows that the green light-emitting phosphor mainly consisted of $Ba_{1.31}Ca_{0.69}SiO_{4}$ (JCPDS $\#$ 36-1449) and other minor phases i.e., $MgSiO_3$ (JCPDS $\#$ 22-0714) and $Ca_{2}BaMgSi_{2}O_{8}$ (JCPDS $\#$ 31-0128). The blue light-emitting phosphor mainly consisted of $Ca_{2}BaMgSi_{2}O_{8}$ phase.

Observation of the Cosmic Near-Infrared Background with the CIBER rocket

  • 김민규;;이형목;;;;;;;;;이대희;;;;;남욱원
    • 천문학회보
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    • 제37권1호
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    • pp.42-42
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    • 2012
  • The First stars (Pop.III stars) in the universe are expected to be formed between the recombination era at z - 1100 and the most distant quasar (z - 8). They have never been directly detected due to its faintness so far, but can be observed as a background radiation at around 1${\mu}m$ which is called the Cosmic Near-Infrared Background (CNB). Main part of the CNB is thought to be redshifted Lyman-alpha from gas clouds surrounding the Pop.III stars. Until now, the COBE (COsmic Background Explorer) and the IRTS (Infrared Telescope in Space) observed excess emission over the background due to galaxies. To confirm the COBE and the IRTS results and pursue more observational evidences, we carried out the sounding rocket experiment named the Cosmic Infrared Background ExpeRiment (CIBER). The CIBER is successfully launched on July 10, 2010 at White Sands Missile Range, New Mexico, USA. It consists of three kinds of instruments. We report the results obtained by LRS (Low Resolution Spectrometer) which is developed to fill the uncovered spectrum around 1${\mu}m$. LRS is a refractive telescope of 5.5 cm aperture with spectral resolution of 20 - 30 and wavelength coverage of 0.7 to 2.0${\mu}m$. After subtracting foreground components (zodiacal light, integrated star light and diffuse galactic light) from the sky brightness of observed five fields, there remained significant residual emission (even for the lower limit case) consistent with the IRTS and the COBE results. In addition, there exists a clear gap at 0.7 - 0.8${\mu}m$ in the CNB spectrum over the background due to galaxies according to recent results (Matsuoka et al. 2011; Mattila et al. 2011). The origin of the excess emission could be ascribed to the Pop.III stars with its active era of z = 7 - 10.

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The Development of Water Quality Monitoring System and its Application Using Satellite Image Data

  • Jang, Dong-Ho;Jo, Gi-Ho
    • 대한원격탐사학회:학술대회논문집
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    • 대한원격탐사학회 1998년도 Proceedings of International Symposium on Remote Sensing
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    • pp.376-381
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    • 1998
  • In this study, we was measured the radiance reflectance by using multi-spectral image of low resolution camera(LRC) which will be loaded in the multi-purpose satellite(KOMPSAT) to use the data in analyzing water pollution. Also we investigated the possibility of extraction of water quality factors in rivers and water body by using high resolution remote sensing data such as Airborne MSS. Especially, we tried to extract the environmental factors related with eutrophication, and also tried to develop the process technique and the radiance feature of reflectance related with eutrophication. The results were summarized as follows: First, the spectrum of sun's rays which reaches the surface of the earth was consistent with visible rays bands of 0.4${\mu}{\textrm}{m}$~0.7${\mu}{\textrm}{m}$ and about 50% of total quantity of radiation were there. And at around 0.5${\mu}{\textrm}{m}$ of green spectral band in visible rays bands, the spectrum was highest. Second, as a result of the radiance reflectance Chlorophyll-a represented high spectral reflectance mainly around 0.52${\mu}{\textrm}{m}$ of green spectral band, and suspended sediments and turbidity represented high spectral reflectance at 0.8${\mu}{\textrm}{m}$ and at 0.57${\mu}{\textrm}{m}$ each. Third, as a result of the water quality analysis by using Airborne MSS, Chlorophyll-a could have a distribution chart when carried out ratio of B3 and BS to B7. And Band 7 was useful for making the distribution chart of suspended sediments. And when we carried out PCA, suspended sediments and turbidity had distributions at PC 1 , PC 4 each similarly to ground truth data. Above results can be changed according to the change of season and time. Therefore, in order to analyze more exactly the environmental factors of water quality by using LRC data, we need to investigate constantly the ground truth data and the radiance feature of reflectance of water body. Afterward in this study, we will constantly analyze the radiance feature of the surface of water in water body by measuring the on-the-spot radiance reflectance and using low resolution satellite image(SeaWiFs). Besides, we will gather the data of water quality analysis in water body and analyze the pattern of water pollution.

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치과 방사선촬영 시 구내 센서 내 차폐체 삽입을 통한 피폭선량 감소 연구 (A Study on the Reduction of Absorbed Dose through the Insertion of a Shielding Material in the Intraoralsensor of Dental Radiography)

  • 김아연;이승재
    • 한국방사선학회논문지
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    • 제16권3호
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    • pp.273-279
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    • 2022
  • 치과 방사선촬영 시 환자에게 부여되는 피폭선량을 감소시키기 위해 구내 센서 내에 차폐체를 삽입하는 센서를 설계하였다. 설계한 센서를 사용하여 차폐체의 사용 유무에 따른 피폭선량의 변화를 평가하였다. 피폭선량 평가에 사용한 시스템은 바텍 사의 VEX-S300C이며, 65 kV, 3 mA, 0.15 sec의 조사 조건을 바탕으로 SPEKTR 시뮬레이션을 통해 X-선의 에너지스펙트럼을 획득하고, 각 에너지별 광자수를 도출하였다. Genat4 Application for Tomographic Emission(GATE) 시뮬레이션을 통해 시스템을 설계한 후 획득한 에너지스펙트럼을 방사선원으로 사용하여 피폭선량을 산출하였다. 차폐체는 납을 사용하였으며, 0.1 mm ~ 0.5 mm까지 0.1 mm 두께 간격으로 시뮬레이션을 수행하였으며, 이때 설계한 조사야는 직경 60 mm와 시스템의 선택 사항으로 사용 가능한 20 mm × 30 mm의 조사야에 대한 피폭선량을 평가하였다. 직경 60 mm 조사야를 사용할 경우 차폐체의 유무에 따른 피폭선량의 감소는 차폐체의 두께가 증가함에 따라 지수함수적으로 감소하였다. 또한 20 mm × 30 mm 조사야를 사용할 경우 차폐체를 사용하지 않았음에도 피폭선량은 상당히 감소하였고, 차폐체를 사용할 경우 더욱 피폭선량은 감소하는 것을 확인할 수 있었다.

6SV2.1과 GK2A AOD를 이용한 기계학습 기반의 Sentinel-2 영상 대기보정 (Machine Learning-based Atmospheric Correction for Sentinel-2 Images Using 6SV2.1 and GK2A AOD)

  • 김서연;윤유정;강종구;정예민;최소연;임윤교;서영민;박찬원;이경도;나상일;안호용;류재현;이양원
    • 대한원격탐사학회지
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    • 제39권5_3호
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    • pp.1061-1067
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    • 2023
  • 이 단보에서는 차세대 중형위성 4호(농림위성)의 활용에 앞서, 농림위성과 분광밴드가 유사한 Sentinel-2 위성영상에 대하여 대기보정을 모의하였다. second simulation of the satellite signal in the solar spectrum - vector(6SV)2.1 복사전달모델과 기계학습의 일종인 랜덤 포레스트(random forest, RF)를 활용하여 6SV2.1을 모사한 RF 기반의 대기보정 모델을 개발한 결과, 6SV2.1로 산출된 반사도와 RF 모델로 예측된 반사도 간의 유사도가 매우 높게 나타났다.

의료방사선 피폭선량 저감을 위한 맞춤형 차폐재 설계에 관한 연구 (The Study on Design of Customized Radiation Protective Layer for Medical Radiation Dose Reduction)

  • 강상식;김교태;노시철;정봉재;박지군
    • 한국방사선학회논문지
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    • 제8권6호
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    • pp.333-338
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    • 2014
  • 최근 의료 분야에서의 불필요한 피폭을 체계적으로 관리해야 한다는 사회적 요구 증가와 더불어 차폐의 중요성이 대두되고 있는 실정이다. 하지만 현재 상용화된 제품은 다양한 의료방사선 분야보다 세분되어 있지 않다. 이에 본 연구에서는 최적화된 차폐재의 구조를 몬테카를로 시뮬레이션을 활용하여 제시하고자 하였다. 모의 추정 결과, 유방촬영 에너지(30 kVp) 스펙트럼에 대하여 단일 차폐재의 경우 $30{\mu}mPb$, 2 mmAl에서 90% 이상의 차폐율을 확인하였고, 이중차폐 구조에서는 0.03 mmPb와 1 mmAl의 설계 시 효율적인 것으로 판단되었다. 또한, 일반촬영 에너지(80 kVp) 스펙트럼에 대해서는 $340{\mu}mPb$, 30 mmAl에서 90% 이상의 차폐율을 확인하였으며, 이중차폐 구조에서는 0.3 mmPb와 1 mmAl의 설계가 유용할 것으로 사료된다. 이러한 결과는 향후 피폭저감을 위한 맞춤형 상용화 제품 개발에 대한 기초자료로 활용될 수 있을 것으로 기대된다.

Radiolabeling of 11C-sertraline by fast and easy loop method with [11C]CH3OTf

  • Lee, Hak Jeong;Jeong, Jae Min;Lee, Sang-Yoon;Ido, Tatsuo
    • 대한방사성의약품학회지
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    • 제3권1호
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    • pp.32-37
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    • 2017
  • Cis-(1S,4S)-4-(3,4-dichlorophenyl)-1,2,3,4-tertrahydro-N-methyl-1-naphthalenamine (sertraline) hydrochloride from among selective serotonin reuptake inhibitors (SSRIs) is a treatment of major depression. For the differential diagnosis by metabolizing serotonin in a patient with neurological disorders, the radiolabeled $^{11}C$-sertraline was developed for non-invasive positron emission tomography in living brain and use the evaluation of new drug for SSRIs. We release the results of a fast and easy radiolabeling method applied a one-step loop method with $[^{11}C]CH_3OTf$ for routine clinical applications of $^{11}C$-sertraline. 1 mg of a precursor for $^{11}C$-sertraline in 0.1 mL DMF and $5{\mu}L$ of 1N NaOH, were injected into the loop of semi-prep high-performance liquid chromatography (HPLC). $[^{11}C]CH_3OTf$ was passed through the loop at room temperature (RT). The $^{11}C$-sertraline was separated by the semi-preparative HPLC. $^{11}C$-sertraline was eluted at 28.0 min was collected and evaluated by analytical HPLC and mass spectrometer. The total radiolabeling efficiency of $^{11}C$-sertraline was $30.7{\pm}8.7%$. The specific activity was $64.8{\pm}51.4GBq/{\mu}mol$. The radiochemical and chemical purities were higher than 99%. The mass spectrum of the product showed m/z peaks at 307.1 (M+1), indicating the mass of sertraline. By the one-step loop method with $[^{11}C]CH_3OTf$, $^{11}C$-sertraline could be quickly and easily prepared for clinical application.

감마선 및 엑스선의 피이크 분석 (Peak Analysis of Gamma-ray and X-ray)

  • 김승곤;허영회;박광준
    • Journal of Radiation Protection and Research
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    • 제9권1호
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    • pp.33-42
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    • 1984
  • 핵분열(核分裂) 및 방사화생성물(放射化生成)物)에서 방출(放出)하는 여러가지 감마선들은 핵연료(核燃料)를 파괴(破壞)하지 않고도 추출(抽出)할 수 있는 많은 정보(情報)를 포함(包含)한다. 그러나 반도체(半導體) 검출기(檢出器)에서 얻은 복잡한 스펙트럼에서 이러한 정보를 추출(抽出)하기가 용역(容易)하지 않기 때문에 전산(電算)코드의 사용(使用)이 필요(必要)하게 된다. 본(本) 연구(硏究)에서는 그동안 국제적(國際的)으로 널리 보급(普及)되어 사용(使用)되는 감마선 분석(分析) 프로그램들의 장점(長點)을 취하여, 감마선은 물론 X-선(線)의 스펙트럼도 피팅 (fitting)하여 피이크의 중심과 면적을 정확(正確)히 계산(計算)할 수 있는 전산코드 CAERI를 개발(開發)하였다. CAERI는 FORTRAN으로 쓰여있고, 특히 고유복사선폭(固有輻射線幅)(natural line width) 을 무시할 수 없는 X-선(線)의 피이크 표현함수(表現函數)인 Voigt 함수(函數)에 대해서는, 다른 X-선(線) 분석(分析) 프로그램들이 사용(使用)한 간단한 근사식(近似式) 대신에, 더욱 정확(正確)한 무한급수근사식(無限級數近似式)을 사용하였다. 특히 CAERI 는 U이나 Pu과 같은 중원소(重元素)의 핵종분석시(核種分析時)에 직면(直面)하는 감마선과 U이나 Pu의 X-선(線)이 임의(任意)로 간섭(干涉)하며 공존(共存)하는 복잡한 스펙트럼까지도 취급(取扱)할 수 있다. $^{177m}Lu$감마선과 $^{235}U\;U_{\alpha}$X-선(線)의 시험(試驗)스펙트럼을 피팅하여, 다른 프로그램들의 피팅결과와 비교했을 때 좋은 일치(一致)를 보았다.

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