• 제목/요약/키워드: total magnetic field

검색결과 199건 처리시간 0.027초

지진 위치와 관련된 지자기장 변동성 분석: 2012년부터 2014년까지 한반도 지역 발생 지진을 중심으로 (An Analysis of Geomagnetic Variations Related to Earthquakes Location which Occurred in and around the Korean Peninsula from 2012 to 2014)

  • 민동민;오석훈;지윤수
    • 한국지구과학회지
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    • 제36권7호
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    • pp.649-660
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    • 2015
  • 2012년부터 2014년까지 한반도 및 그 주변에서 일어난 지진과 지자기장 변동성과의 상관관계를 연구하였다. 웨이블릿 기반의 셈블런스 분석기술을 지진과 관련된 지자기장 변동성 분석에 사용하였다. 총자기장을 이용한 분석 결과 관측소 반경 100 km 이내에서 발생한 지진의 경우 일관적인 셈블런스 변동양상이 나타남을 확인하였고, Z축 성분 지자기장 자료를 이용한 웨이블릿 기반의 셈블런스 분석에서도 비슷한 변동양상을 확인하였다. 자료 질이 좋은 청양 관측소 지자기장 자료를 중심적으로 분석하였고, 추가적으로 보현산 관측소의 Z축 성분 자료를 해석하여 상관성에 대한 신뢰도를 확인하고자 하였다.

Prophylactic extended-field irradiation with concurrent chemotherapy for pelvic lymph node-positive cervical cancer

  • Oh, Jinju;Seol, Ki Ho;Lee, Hyun Joo;Choi, Youn Seok;Park, Ji Y.;Bae, Jin Young
    • Radiation Oncology Journal
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    • 제35권4호
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    • pp.349-358
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    • 2017
  • Purpose: This study aimed to evaluate whether prophylactic extended-field pelvic radiotherapy (EF-PRT) yields better results than standard whole pelvic radiotherapy (WPRT) in patients with pelvic lymph node-positive cervical cancer treated with concurrent chemoradiotherapy (CCRT). Materials and Methods: A total of 126 cases of stage IB-IVA cervical cancer that had pelvic lymph node involvement in magnetic resonance imaging and were treated with CCRT between 2000 and 2016 were reviewed. None of the patients had para-aortic lymph node (PALN) metastases. The patients were classified to two groups, namely, those treated with EF-PRT, including prophylactic para-aortic radiotherapy, and those treated only with WPRT. The median dose to the PALN area in patients treated with EF-PRT was 45 Gy. All patients received concurrent cisplatin-based chemotherapy. Results: Overall, 52 and 74 patients underwent EF-PRT and WPRT, respectively. Patient characteristics and irradiated dose were not significantly different, except the dose to the para-aortic area, between the two groups. The median follow-up period was 75.5 months (range, 5 to 195 months). The 10-year cumulative recurrence rate of PALN for EF-PRT vs. WPRT was 6.9% and 10.1% (p = 0.421), respectively. The 10-year disease-free survival and overall survival for EF-PRT vs. WPRT were 69.7% vs. 66.1% (p = 0.748) and 71.7% vs. 72.3% (p = 0.845), respectively. Acute gastrointestinal complications were significantly higher in EF-PRT (n = 21; 40.4%) than WPRT (n = 26; 35.1%) (p = 0.046). Late toxicities were not significantly different in both groups. Conclusion: In this study, prophylactic radiotherapy for PALN does not have an additional benefit in patients with pelvic lymph node-positive cervical cancer treated with CCRT.

고위도 하부 열권 바람의 소용돌이도와 발산 분석: 행성간 자기장(IMF)에 대한 의존도 (Analysis of Wind Vorticity and Divergence in the High-latitude Lower Thermosphere: Dependence on the Interplanetary Magnetic Field (IMF))

  • 곽영실;이재진;안병호;황정아;김관혁;조경석
    • Journal of Astronomy and Space Sciences
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    • 제25권4호
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    • pp.405-414
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    • 2008
  • 이 연구에서는 고위도 하부 열권 역학을 좌우하는 물리적 과정을 이해하기 위하여, 상이한 행성간 자기장(Interplanetary Magnetic Field, IMF)에 따른 남반구 고위도 하부 열권에서의 소용돌이도(vorticity)와 발산(divergence)을 분석하였다. 이 연구를 위하여 미국립대기연구소(National Center for Atmospheric Research, NCAR)의 열권-이온권 전기역학적 대순환 모델(Thermo sphere-Ionosphere Electrodynamic General Circulation Model, TIEGCM)을 이용하였다. 소용돌이도와 발산 분석은 전체 수평 바람장을 최종적으로 결정하는 운동량원(momentum source)을 밝히는데 도움을 주는 근원적인 흐름을 파악할 수 있게 해주며, 운동량원들의 상대적인 강도를 분석해내는데 좋은 도구가 된다. 고위도 하부 열권의 평균 바람장은 태양 복사와 쥴가열에 의해 유발되는 발산운동 보다는 이온대류에 의해 유발되는 회전운동에 의해 주로 지배된다는 것이 확인되었다. $IMF{\neq}0$와 IMF=0인 경우의 고위도 열권 하부에서의 소용돌이도 차이(difference vorticity)가 모든 IMF 조건에서 발산장 차이(difference divergence)에 비해 훨씬 더 크게 나타났다. 이는 IMF가 발산적인 흐름보다 회전적인 흐름에 더 강하게 영향을 끼치며, 나아가 IMF가 발산운동을 유발하는 에너지 유입보다는 회전운동을 유발하는 운동량 유입에 더 강하게 영향을 끼침을 의미한다. IMF의 방향에 따라 고위도 하부 열권에서의 소용돌이도 차이의 양상이 매우 달랐다 $B_y$가 음일 때는 지자기 위도 $-70^{\circ}$ 이상의 고위도에서 극을 중심으로 양의 소용돌이도 차이가 나타나고 $B_y$가 양일 때는 음의 소용돌이도 차이가 나타났다. $B_z$가 음인 경우 소용돌이도 차이가 저녁 영역에는 양이고 새벽 영역에는 음이며, $B_z$가 양인 경우에는 반대의 분포를 보였다. $B_z$가 음일 때가 양일 때보다 소용돌이도 차이가 더 큰 것으로 확인되었는데, 이는 IMF $B_z$가 남쪽으로 향할 때가 북쪽으로 향할 때보다 고위도 이온권의 이온대류를 더 강화시켜 열권 중성대기의 회전적인 흐름을 더 강하게 유발시킴을 의미한다.

의성지역 백악기 암석에 대한 고자기 연구 (Palaeomagnetism of Cretaceous Rocks in the Ǔisǒng Area, Kyǒngsang Basin, Korea)

  • 김인수;이현구;윤혜수;강희철
    • 자원환경지질
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    • 제26권3호
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    • pp.403-420
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    • 1993
  • The Cretaceous Kyongsang Basin is known to be composed of several tectonic blocks (or subbasins) with each distinct stratigraphic succession. The study area represents a major part of one of these blocks, i. e. the $\check{U}is\check{o}ng$ block. The area is charaterized by a suite of WNW-trending sinistral strike-slip faults as well as a number of ring faults. A total of 292 independently oriented core samples were drilled from 23 sites, covering virtually all the formations of the Cretaceous $Ky\check{o}ngsang$ Supergroup. Alternating field and thermal demagnetization experiments were conducted to reveal the primary magnetization. Due to the homoclinal nature of the strata in the area, it was not possible to make use of the conventional fold test It is, however, believed that the primary remanent components have been obtained from the majority of the formations, considering the similarity of the palaeomagnetic pole positions with those of contemporary strata of other blocks and the existence of antiparallel reversed remanence. It was found neither any significant difference in magnetic declination on each side of the strike-slip faults nor systematic change of magnetic declination with distance from the fault-line. This does not support such a block rotation hypothesis associated with the strike-slip faulting in the area as alleged by some authors. The samples from the outcrops on or near the fault-lines were severely overprinted by the recent magnetic fields regardless of age and lithology. Epithermal Au-Ag-Cu-Pb-Zn mineralizations are known along some fault lines in the area. It is interpreted that these two facts are closely related with fluid circulations along the fracture zones caused by fault activities. In regard to the age of the strata as deduced from the magnetostratigraphic consideration, the $Ch\check{o}mgok$ formation and the lower strata should be older than Barremian or 124 Ma. The age of volcanics of the $Yuch^{\prime}\check{o}n$ Group sampled in this study should be younger than Campanian or 83 Ma.

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Magnetic Resonance Imaging Patterns of Post-Operative Spinal Infection : Relationship between the Clinical Onset of Infection and the Infection Site

  • Kim, Seon-Jeong;Lee, Sang Hoon;Chung, Hye Won;Lee, Min Hee;Shin, Myung Jin;Park, Seoung Woo
    • Journal of Korean Neurosurgical Society
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    • 제60권4호
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    • pp.448-455
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    • 2017
  • Objective : To investigate the magnetic resonance imaging (MRI) findings and the patterns of postoperative spinal infection according to the passage of time. Methods : Institutional review board approval was obtained, and informed consent was not obtained for the retrospective review of patients' medical records. A total of 43 patients (27 men and 16 women; mean age, 64) diagnosed with postoperative spinal infection were included in this study. We retrospectively reviewed the MRI findings and the medical records and categorized the infection sites based on MRI, i.e., anterior, posterior, and both parts. The duration of the clinical onset from surgery was divided, i.e., acute (${\leq}2weeks$), subacute (2-4 weeks), and late (>4 weeks). Results : Postoperative spinal infection was involved in the posterior part in 31 (72%), anterior part in two (4.7%), and both parts in 10 patients (23.3%). Abscess or phlegmon in the back muscles and laminectomy site were the most common MRI findings. The number of patients with acute, subacute, and late clinical onset were 35, two, and six, respectively (mean, 33.4 days; range, 1-730 days). The mean duration of the clinical onset was 12 days in the posterior part, 15.2 days in both parts, and 456.5 days in the anterior part. Conclusion : Postoperative spinal infection usually occurred within four weeks in the posterior part and over time the infection was considered to spread into the anterior part. For the evaluation of postoperative spinal infection, the posterior surgical field was more important than the vertebral body or the disc space on MRI.

Technical Feasibility of Quantitative Measurement of Various Degrees of Small Bowel Motility Using Cine Magnetic Resonance Imaging

  • Ji Young Choi;Jihye Yun;Subin Heo;Dong Wook Kim;Sang Hyun Choi;Jiyoung Yoon;Kyuwon Kim;Kee Wook Jung;Seung-Jae Myung
    • Korean Journal of Radiology
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    • 제24권11호
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    • pp.1093-1101
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    • 2023
  • Objective: Cine magnetic resonance imaging (MRI) has emerged as a noninvasive method to quantitatively assess bowel motility. However, its accuracy in measuring various degrees of small bowel motility has not been extensively evaluated. We aimed to draw a quantitative small bowel motility score from cine MRI and evaluate its performance in a population with varying degrees of small bowel motility. Materials and Methods: A total of 174 participants (28.5 ± 7.6 years; 135 males) underwent a 22-second-long cine MRI sequence (2-dimensional balanced turbo-field echo; 0.5 seconds per image) approximately 5 minutes after being intravenously administered 10 mg of scopolamine-N-butyl bromide to deliberately create diverse degrees of small bowel motility. In a manually segmented area of the small bowel, motility was automatically quantified using a nonrigid registration and calculated as a quantitative motility score. The mean value (MV) of motility grades visually assessed by two radiologists was used as a reference standard. The quantitative motility score's correlation (Spearman's ρ) with the reference standard and performance (area under the receiver operating characteristics curve [AUROC], sensitivity, and specificity) for diagnosing adynamic small bowel (MV of 1) were evaluated. Results: For the MV of the quantitative motility scores at grades 1, 1.5, 2, 2.5, and 3, the mean ± standard deviation values were 0.019 ± 0.003, 0.027 ± 0.010, 0.033 ± 0.008, 0.032 ± 0.009, and 0.043 ± 0.013, respectively. There was a significant positive correlation between the quantitative motility score and the MV (ρ = 0.531, P < 0.001). The AUROC value for diagnosing a MV of 1 (i.e., adynamic small bowel) was 0.953 (95% confidence interval, 0.923-0.984). Moreover, the optimal cutoff for the quantitative motility score was 0.024, with a sensitivity of 100% (15/15) and specificity of 89.9% (143/159). Conclusion: The quantitative motility score calculated from a cine MRI enables diagnosis of an adynamic small bowel, and potentially discerns various degrees of bowel motility.

확장된 Born 근사에 의한 시추공간 전자탐사 2.5차원 모델링 (Crosshole EM 2.5D Modeling by the Extended Born Approximation)

  • 조인기;서정희
    • 지구물리와물리탐사
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    • 제1권2호
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    • pp.127-135
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    • 1998
  • 전자탐사에서 Born 근사는 이상체내에서의 전기장을 이상체가 없는 균질 매질에서의 일차장으로 대치하는 방법으로 복잡한 전자기 산란(EM scattering)문제를 근사하는데 널리 사용되고 있는 방법이다. 그러나 Born 근사는 이상체의 전도도가 주변 매질에 비하여 너무 크거나, 이상체의 크기가 클 때는 상당히 부정확한 결과를 나타낸다. 확장된 Born근사법은 이러한 Born근사의 문제점을 해결하기 위하여 제안된 방법으로 이상체내의 전기장을 탈분극 텐서와 일차 전기장의 곱으로 근사하는 방법이다. 한편 전자탐사에 3차원 송신원을 사용하는 2차원 모델링은 주로 유한차분법과 유한요소법이 이용되었다. 일반적으로 이들 미분 방정식을 이용하는 2차원 전자탐사 모델링에서 3차원 송신원 문제의 해결을 위하여 Fourier변환을 통해 파수영역(wavenumber domain)으로 이동하는 방법이 사용되어 왔다. 또한 파수영 역에서 계산된 결과는 Fourier 역변환을 통하여 다시 공간영역(space domain)으로 이동해야 하는 번거로움이 있다. 따라서 이들 방법은 계산시간이 많이 걸리고 이상체가 없는 지역도 미소체로 분할해야 하므로 수치계산시 대량의 기억용량이 필요하다. 본 연구에서는 Born근사의 문제점 및 전자탐사 2차원 모델링시 3차원 송신원 문제를 해결할 수 있는 확장된 Born 근사법에 근거한 전자탐사 2.5차원 모델링 프로그램을 개발하였다. 이 모델링 프로그램을 이용하여 수직 자기 쌍극자를 송신원으로 하는 시추공간 전자탐사법에 대한 2차 자기 장을 계산하고 적분 방정식에 의한 3차원 모델링 결과와 비교, 분석하였다. 모든 주파수 대역에서 확장된 Born근사에 의한 2.5차원 모델링 결과가 3차원 모델링 결과와 잘 일치하고 있다. 그러나 이상체의 전도도와 모암의 전도도 차이가 10배 이상의 경우일 때는 두 반응은 상당한 차이를 보인다. 따라서 본 연구에서 개발된 확장된 Born 근사에 의한 2.5차원 모델링은 이상체와 모암의 전도도 차이가 너무 크지 않을 경우 이상체의 위치 및 형상을 파악하는데 효과적일 것으로 기대된다.

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슬관절 전치환술 후 기능 회복을 위한 치료법 (Treatment Methods for Functional Recovery after Total Knee Arthroplasty)

  • 김영모;주용범;박일영
    • 대한정형외과학회지
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    • 제55권2호
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    • pp.117-126
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    • 2020
  • 슬관절의 퇴행성 관절염에서 슬관절 전치환술은 널리 시행되고 있고 그 빈도도 점점 증가되고 있다. 수술 후 일상생활로의 복귀, 근력 및 운동범위의 회복 등 기능 회복을 위한 노력이 이루어져야 하고 이는 환자 요인, 수술 술기 및 재활 등 다양한 관점에서 접근해야 한다. 환자의 연령이나 비만의 정도, 성별, 대퇴사두근의 근력 등이 수술 후 기능 회복에 영향을 줄 수 있고 환자의 기대치나 만족도 같은 정신적인 상태도 영향을 준다. 기능 회복을 위하여 수술 전부터 환자교육 및 통증 조절, 대퇴사두근 근력의 강화 같은 치료를 시행할 수 있다. 수술 후 냉찜질 및 압박, 경피적 전기 신경 자극 치료, 신경근육 전기 자극 치료, 저주파 저강도 자기장 치료, 대퇴사두근의 근력운동, 관절범위 운동과 같은 물리치료도 적용할 수 있다. 최근에는 수중에서 근력과 균형감각을 회복시키는 수 치료도 점점 시행되는 추세이다. 이런 기능 회복을 위한 치료들은 수술 후 단기적으로만 시행될게 아니라 장기적으로 꾸준히 시행되는 것이 중요하며 술자는 환자의 상태나, 순응도, 사회적, 심리적 상황 등을 고려하여 적절히 적용하여야 한다.

남녀 및 나이에 따른 심자도 변수 차이 분석 (Analysis of the Parameters of Magnetocardiography Depending on the Age and Gender)

  • 임현균;정남식;이용호;권혁찬;정보영;박용기
    • 대한의용생체공학회:의공학회지
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    • 제28권4호
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    • pp.530-538
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    • 2007
  • Magnetocardiography (MCG) is a device to measure the magnetic field from the heart. It is a noninvasive device and takes only few minutes to record magnetocardiogram from a subject. In this study, we compared the difference of MCG data recorded from 56 normal subjects in early twenties (28 males and 28 females, mean $age=21.0{\pm}1.6$ years) and 36 elderly subjects (20 males and 16 females, mean $age=61.9{\pm}6.9$ years) for the analysis of the age and gender difference. A total of 24 parameters used in the analysis were derived from QRS complex, R-wave, T-wave, and ST-T period. As a result, seven parameters including maximum current angle and map angle showed the significant difference (p<0.01 and p<0.05, respectively) between young males and young females. Significant difference (p<0.05) between elderly males and elderly females was found from a parameter, pole distance at T-wave peak. In the comparison of age difference, seven parameters regarding current moment, pole distance, and dynamics showed the significant difference between young and elderly males. Eight parameters also showed significant difference (p<0.05) between two younger and elderly female groups. Results showed that parameters regarding current moment, pole distance, and dynamics might be changed when people get older. In conclusion, gender and age difference should be considered when MCG data are analyzed for certain parameters.

INTRINSIC BRIGHTNESS TEMPERATURES OF COMPACT RADIO JETS AS A FUNCTION OF FREQUENCY

  • Lee, Sang-Sung
    • 천문학회지
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    • 제47권6호
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    • pp.303-309
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    • 2014
  • We present results of our investigation of the radio intrinsic brightness temperatures of compact radio jets. The intrinsic brightness temperatures of about 100 compact radio jets at 2, 5, 8, 15, and 86 GHz are estimated based on large VLBI surveys conducted in 2001-2003 (or in 1996 for the 5 GHz sample). The multi-frequency intrinsic brightness temperatures of the sample of jets are determined by a statistical method relating the observed brightness temperatures with the maximal apparent jet speeds, assuming one representative intrinsic brightness temperature for a sample of jets at each observing frequency. By investigating the observed brightness temperatures at 15 GHz in multiple epochs, we find that the determination of the intrinsic brightness temperature for our sample is affected by the flux density variability of individual jets at time scales of a few years. This implies that it is important to use contemporaneous VLBI observations for the multi-frequency analysis of intrinsic brightness temperatures. Since our analysis is based on the VLBI observations conducted in 2001-2003, the results are not strongly affected by the flux density variability. We find that the intrinsic brightness temperature $T_0$ increases as $T_0{\propto}{\nu}^{\xi}_{obs}$ with ${\xi}=0.7$ below a critical frequency ${\nu}_c{\approx}9GHz$ where the energy loss begins to dominate the emission. Above ${\nu}_c$, $T_0$ decreases with ${\xi}=-1.2$, supporting the decelerating jet model or particle cascade model. We also find that the peak value of $T_0{\approx}3.4{\times}10^{10}$ K is close to the equipartition temperature, implying that the VLBI cores observable at 2-86 GHz may be representing jet regions where the magnetic field energy dominates the total energy in jets.