• Title/Summary/Keyword: Disk Imaging

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Dynamo Test Research for Performance Verification of CV-NCM Cast Iron Brake Disk (CV-NCM 주철재 제동디스크의 성능 검증을 위한 다이나모 시험연구)

  • Gil, Hyeong-Gyeun;Ko, Tae-Whan;Cho, Dong-Hyun;Han, Seong-Ho
    • Proceedings of the KSR Conference
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    • 2006.11b
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    • pp.274-280
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    • 2006
  • The study is to analyze dynamo test results for various commercial pads in order to verify the performance of brake disk with CV-NCM cast iron. The developed brake disk will apply to 200 km/h tilting trains that is being developed as one part of project for speed-up on Korean existing railroad. The test program is made out suitably for braking condition and performance of test equipment by referring UIC 541-3. Two kinds of resin pad and one kind of foreign sintered pad suitable for 200 km/h trains are used as various commercial pad for the dynamo test. The data aquisition for the maximum and smallest temperature, hot spot, etc. on disk and pad is performed by using the thermocouples and thermal imaging cameras. From this research, we obtained braking characteristics between CV-NCM cast iron disk and pad of various material and will be utilized usefully as basis data of performance optimization of developing sintered pad.

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Condylar position on the lateral individualized corrected tomography in internal derangement of temporomandibular joint (측두하악관절 내장증시 측방 개별화 보정단층방사선사진에서의 하악과두의 위치)

  • Kim Keun-Min;Hwang Eui-Hwan;Lee Sang-Rae
    • Imaging Science in Dentistry
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    • v.32 no.2
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    • pp.67-73
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    • 2002
  • Purpose: To examine the possible relationship between condylar position and disk displacement in the temporomandibular joint. Materials and Methods: 79 temporomandibular joints in 40 patients having temporomandibular disorders were classified into three categories: no disk displacement (NDD) , disk displacement with reduction (DDWR), and disk displacement without reduction (DDWOR). Disk positions were assessed from clinical and MRI findings. The relationship between the three categories and condylar positions was evaluated using lateral individualized corrected tomography. Results: Clinical findings regarding the relationship between condyle and disk positions having anterior, centric, and posterior positions were 27%, 27%, and 46%, respectively, in NDD, 43%, 17%, and 40%, respectively, in DDWR, and 44%, 22%, and 34%, respectively, in DDWOR. There were no significant differences in condylar positions between each of the groups (P>0.05). In the relationship between condyle and disk positions with MRI findings, anterior, centric, and posterior positions were 38%, 38%, and 24%, respectively, in NDD, 29%, 21%, and 50%, respectively, in DDWR, and 44%, 9%, and 47% respectively, in DDWOR. There were significant differences in the condylar positions when MRI was utilized (P<0.05) Conclusion: There was a significant correlation between the condyle and disk positions with MRI findings on lateral individualized corrected tomography.

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The WSRT HI Imaging Study of Gas-rich Galaxies in the Outskirts of the Virgo Cluster

  • Yoon, Hyein;Chung, Aeree;Sengupta, Chandreyee;Wong, O. Ivy;Bureau, Martin;Rey, Soo-Chang;van Gorkom, J.H.
    • The Bulletin of The Korean Astronomical Society
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    • v.40 no.1
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    • pp.76.2-76.2
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    • 2015
  • We present the results of the Westerbork Synthesis Radio Telescope (WSRT) HI imaging study of seven late-type galaxies. They are located in the outskirts of the Virgo cluster, possibly along a filament connected to Virgo from the north-west. Most galaxies in this region are found to be HI-rich, containing more HI gas compared to field galaxies with similar size and optical luminosity. The positions of the sample with respect to the cluster and their high HI mass-to-light ratios suggest that the selected galaxies might be accreting more gas from their surroundings while falling into the cluster. By high-resolution HI imaging, we aim to find evidence that galaxies are pre-processed by gas accretion from the intergalactic medium and/or gas-rich neighbors. We probe the detailed HI morphology/kinematics and the star formation properties of the sample. All of these galaxies are found with a large HI disk which is quite extended compared to their stellar disk. Together with kinematical peculiarities, this strongly suggests that cold gas accretion is responsible for active star formation in these galaxies.

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Comparison of static MRI and pseudo-dynamic MRI in tempromandibular joint disorder patients (측두하악관절장애 환자에서의 static MRI와 pseudo-dynamic MRI의 비교연구)

  • Lee, Jin-Ho;Yun, Kyoung-In;Park, In-Woo;Choi, Hang-Moon;Park, Moon-Soo
    • Imaging Science in Dentistry
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    • v.36 no.4
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    • pp.199-206
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    • 2006
  • Purpose: The purpose of this study was to evaluate comparison of static MRI and pseudo-dynamic (cine) MRI in temporomandibular joint (TMJ) disorder patients. Materials and Methods: In this investigation, 33 patients with TMJ disorders were examined using both conventional static MRI and pseudo-dynamic MRI. Multiple spoiled gradient recalled acquisition in the steady state (SPGR) images were obtained when mouth opened and closed. Proton density weighted images were obtained at the closed and open mouth position in static MRI. Two oral and maxillofacial radiologists evaluated location of the articular disk, movement of condyle and bony change respectively and the posterior boundary of articular disk was obtained. Results: No statistically significant difference was found in the observation of articular disk position, mandibular condylar movement and posterior boundary of articular disk using static MRI and pseudo-dynamic MRI (P<0.05). Statistically significant difference was noted in bony changes of condyle using static MRI and pseudo-dynamic MRI (P<0.05). Conclusion: This study showed that pseudo-dynamic MRI didn't make a difference in diagnosing internal derangement of TMJ in comparison with static MRI. But it was considered as an additional method to be supplemented in observing bony change.

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A Retrospective Study of Intervertebral Disk Disease Confirmed by MRI in Dogs: 89 Cases (2012-2015)

  • Kim, Dam;Kang, Jin-su;Kim, Young-ung;Lee, Dong-bin;Heo, Su-young;Kim, Nam-soo
    • Journal of Veterinary Clinics
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    • v.36 no.3
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    • pp.139-144
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    • 2019
  • Intervertebral disk disease is a common neurological disease in dogs. In veterinary neurology clinics, the incidence of intervertebral disk disease and the spinal cord compression rate of the disk are well documented. However, the direction of herniation of the intervertebral disk is relatively less known on Magnetic resonance imaging (MRI). Therefore, this study systematically investigated and analyzed the intervertebral disk disease in dogs. Especially, classification according to the direction of herniation of the disk, the degree of pre - treatment neurological manifestation, and the compression rate was investigated. In addition, the treatment methods of patients who received treatment after visiting the Chonbuk animal medical center (CAMC) were divided into pharmacological treatment and surgical treatment. The location of intervertebral disc in spinal canal was mainly ventral (69.9%), and when the prognosis was evaluated according to the compression rate of the spinal cord, the prognosis of the surgical treatment (72.7%) was more effective than the non - surgical medication (40.6%). Surgical treatment (83.3%) was more successful than nonsurgical medication (60%), especially in cases of severe spinal cord compression (> 50%). In this study, surgical treatment was more effective when the neurological symptoms were severe or the spinal cord compression rate was high.

Wide-orbit companion candidates and Stellar Disk around T-Tauri Star

  • Oh, Daehyun;Tamura, Motohide
    • The Bulletin of The Korean Astronomical Society
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    • v.39 no.2
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    • pp.86.1-86.1
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    • 2014
  • Two substellar companion candidates with planetary mass, around a T-Tauri star in the ${\rho}$ Ophiuchi star-forming region, are discovered by results of Subaru Telescope's near-infrared imaging. Candidates are separated by 1400au and 500au. If these candidates were real companions, they are the widest-orbit and the lowest mass planetary-mass companions(PMCs) candidates. This discovery may suggest that PMCs form via extreme case of cloud core fragmentation for multiple stars. And also stellar disk are imaged by HiCIAO, hight contrast instrument for exoplanets and disks, with Subaru Telescope. This could be the first case, which imaged both of planetary mass companions and disk around same star. Even two companions candidates are not bounded around the star, they still could be one of the lowest mass objects. In this presentation, I will discuss about observations and confirmations of these objects, and the latest results about their properties.

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Morphologic and positional assessment of temporomandibular joint disk in facial asymmetric patients by magnetic resonance imaging (자기 공명 영상을 이용한 안면비대칭환자의 측두하악관절원반의 형태와 위치에 관한 연구)

  • Zou, Bingshuang;Kim, Tae-Woo;Choi, Soon-Chul
    • The korean journal of orthodontics
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    • v.35 no.5 s.112
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    • pp.398-407
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    • 2005
  • The present study was conducted to examine the morphometrics and function of the disk on both sides among patients with facial asymmetry (FA) and to elucidate plausible correlations between internal derangement (ID) and FA. The sample was composed of 10 males and 27 females with FA. The disk status of all subjects was evaluated by bilateral high resolution magnetic resonance scans in the sagittal (closed and open) and coronal (closed) planes. Five types of disk displacement were identified accordingly. The disk function was diagnosed as normal disk function, disk displacement with reduction, and disk displacement without reduction. The disk shape on sagittal MRI in closed position was classified as bi-concave, biplanar, funnel/hemiconvex, and deformed. The disk position, translation and rotation were also measured. The difference between the shifted side and non-shifted side was analyzed by statistical analysis. Approximately $70\%$ of the patients in the present study showed unilateral or bilateral ID. It was found that anterior disk displacements (ADD), especially rotational ADD, occurred more frequently in the shifted side, while normal disk position was observed mainly in the non-shifted side (p<0.01). The disk of the shifted side showed significantly deformed configuration and inferior-anterior disk position. However, the disk of the non-deviated side showed hyper-mobility during jaw opening movement. These results demonstrate that in FA patients, the disks status of the shifted side is different from that of the non-shifted side, a phenomenon that could be correlated to facial asymmetry.

A STUDY ON THE CHANGES OF MR SIGNAL INTENSITY OF POSTERIOR ATTACHMENT OF THE TEMPOROMANDIBULAR JOINT (악관절 후방부착부에 있어서 MRI 신호변화에 대한 고찰)

  • Jung, Joo-Sung;Huh, Won-Shil;Chung, Hoon
    • Maxillofacial Plastic and Reconstructive Surgery
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    • v.19 no.1
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    • pp.93-107
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    • 1997
  • Magnetic resonance imaging has been used in the temporomandibular joint(TMJ) primarily to define morphology and positional relationship of associating structures. This report examines signal intensity characteristics of the posterior attachment as they related to the severity of internal derangement. Fifty six joints in 35 patients with a history of TMJ dysfunction were imaged writ MR using $T_1$-weighted spin echo sequence. According to disk position, ability to reduction, and the presence of osteoarthritis, the joints were categorized into three groups. A group 1 was anterior disk displacement with reduction; a group 2 was anterior disk displacement without reduction; a group 3 was anterior disk displacement without reduction and condyle had osteoarthritic change. The control group was determined by the clinical absence of any signs or symptoms of current or past TMJ pain and dysfunction. Calculated the relative value of MR signal intensity in posterior attachment and disk to cerebral cortex of temporal lobe by means of computer program, we have compared them with each groups. The result showed statistically little significant difference of disk signal intensity among each groups. but, signal intensity from posterior attachment in group 2 and 3 were significantly(p<0.05) decreased than control group. this might reflect an fibrosis or hyalinization of posterior attachment, which was part of remodeling process that occurs in disk displacement without reduction. However, this study could not demonstrate histologic confirmation of the decreased signal intensity in the posterior attachment. So, further investigation could be needed to understand the association between them.

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Effect of Cervical Spinal Decompression on the Cervical Muscle Tone and Disc Height in Patients with Cervical Intervertebral Disc Herniation

  • Kang, Jeong il;Jeong, Dae Keun;Choi, Hyun
    • Journal of International Academy of Physical Therapy Research
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    • v.9 no.1
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    • pp.1420-1425
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    • 2018
  • The purpose of this study was to investigate the effect of traction and decompression therapies on the cervical muscle tone and disc height. The decompression group (n=16) received decompression therapy and Mckenzie exercises once a day and four times a week respectively, for three weeks. The traction group (n=15) also received traction therapy and Mckenzie exercises for the same period. Muscle tone was measured with a myotonometer, and the disk height was measured using magnetic resonance imaging (MRI), before the interventions. Three weeks later, we investigated the therapeutic effect by repeating these measurements. The difference in disk height between the two groups was not significant. There was a significant difference in the disk herniation index (p<.05). A significant difference was found only in the upper trapezius muscle after comparison of muscle tone and stiffness between the groups (p<.05). Findings from this study suggest that the decompression therapy is a more effective intervention for patients with cervical intervertebral disc herniation.

The Chemical Abundances of Hypervelocity Stars in the Milky Way Disk

  • Yeom, Bum-Suk;Lee, Young Sun;Kim, Young Kwang;Han, Doo-Ri
    • The Bulletin of The Korean Astronomical Society
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    • v.41 no.1
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    • pp.77.2-77.2
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    • 2016
  • We present preliminary results of the analysis of chemical abundances for seven hypervelocity star (HVS) candidates. These objects are G and K dwarfs in the Galactic disk selected from the Sloan Extension for Galactic Understanding and Exploration. Unlike other HVSs discovered thus far, their stellar orbits and kinematics suggest that they do not originate in the Galactic center or in an accretion event. These factors imply yet-unknown mechanisms that give rise to these kinematically-extreme disk stars. In order to study in detail their progenitors and possible formation mechanisms, we obtained spectra of these stars at a resolving power of R~6000, with the Dual Imaging Spectrograph at the Apache Point Observatory. We derive the abundances of chemical elements, C, Mg, Ca, Ti, Cr, Fe, and Ba from the observed spectra, using MOOG. We compare them with the ones of typical Galactic disk stars and discuss discrepancies between them to search for clues to their origin.

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