• Title/Summary/Keyword: Park Disk

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Development of Simulator using RAM Disk for FTL Performance Analysis (RAM 디스크를 이용한 FTL 성능 분석 시뮬레이터 개발)

  • Ihm, Dong-Hyuk;Park, Seong-Mo
    • Journal of the Institute of Electronics Engineers of Korea CI
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    • v.47 no.5
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    • pp.35-40
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    • 2010
  • NAND flash memory has been widely used than traditional HDD in PDA and other mobile devices, embedded systems, PC because of faster access speed, low power consumption, vibration resistance and other benefits. DiskSim and other HDD simulators has been developed that for find improvements for the software or hardware. But there is a few Linux-based simulators for NAND flash memory and SSD. There is necessary for Windows-based NAND flash simulator because storage devices and PC using Windows. This paper describe for development of simulator-NFSim for FTL performance analysis in NAND flash. NFSim is used to measure performance of various FTL algorithms and FTL wear-level. NAND flash memory model and FTL algorithm developed using Windows Driver Model and class for scalability. There is no need for another tools because NFSim using graph tool for data measure of FTL performance.

A Comparison of the Spread Level of the Cervical Epidural Block in Terms of Volume (경부 경막외 차단 시 약물의 용량에 따른 분포 양상 비교)

  • Jo, Dae hyun;Kim, Myoung hee;Ahn, Sun Yeon;Park, Sa Hyun;Lee, Kang Chang
    • The Korean Journal of Pain
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    • v.20 no.1
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    • pp.46-49
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    • 2007
  • Background: Cervical epidural injection, performed via the interlaminar approach, represents a useful interventional pain management procedure indicated in patients with a cervical herniated disk. Due to thedecreased epidural space in the cervical region, cervical epidural injections may result in potentially serious complications, especially during a large volume injection. Methods: Thirty-four patients with neck pain due to a cervical herniated disk that were referred to the pain clinic for cervical epidural steroid injection were randomized into two groups. One group received a cervical epidural injection of 4 ml drug and the other group received 2 ml drug. The injected mixture included triamcinolon, ropivacaine and omnipaque. Spread levels of the drug after injection were estimated with the use of C-arm fluoroscopy. Results: Spread levels to the cephalad for patients in the two groups were $4.88{\pm}0.78segments$ and $4.53{\pm}0.49segments$, respectively. Spread levels to the caudad for patients in the two groups were $4.59{\pm}0.93segments$ and $4.47{\pm}0.51segments$, respectively. The results showed no significant difference in the spread level between the two groups. Conclusions: Use of a small volume of drug (2 ml) can provide a sufficient spread level of the injected drug that is desirable for patients with a cervical herniated disk.

A Study Vertical Surface Discharge Characteristics of the Shape Change of the Solid Insulation with the Same Creepage Distance of Dry-Air (Dry-Air 중의 동일 연면거리를 가진 고체절연물의 형상 변화에 따른 수직연면방전 특성 연구)

  • Jeon, Jong-Cheul;Choi, Byung-Ju;Bae, Sung-woo;Lee, Kwang-Sik;Park, Won-Zoo
    • Journal of the Korean Institute of Illuminating and Electrical Installation Engineers
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    • v.30 no.1
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    • pp.72-78
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    • 2016
  • In terms of power components which use environmentally-friendly dry air that can substitute SF6, there have been studies on the electrical properties of the solid insulation "spacer" for the purpose of securing dielectric strength as they become smaller. This study laminated solid insulation to keep the creeping distance the same in the dry air and investigated vertical surface discharge characteristics by shape. The three sheets of disk-type solid insulation(Bakelite) were laminated in a manner to keep the creeping distance the same. The lamination was categorized as follows: "Type A" in which the insulations with the same disk diameter were laminated; "Type B" in which the insulations whose middle disk diameter was large were laminated; and "Type C" in which the ones whose middle disk diameter was small were laminated. For a vertical surface discharge experiment, dry air was injected into the test chamber depending on the shape of the laminated solid insulation, and chamber pressure was adjusted in a range of 0.1-0.6MPa. As volume decreased, surface discharging voltage by unit volume increased. This was because of dielectric polarization according to the structural characteristics of the shape of lamination. The highest surface discharging voltage was found in "Type C."

Retrieval Policy based on user Classes in Video Sewer (비디오서버에서 사용자 등급을 고려한 검색정책)

  • Kim, Kun-Hyung;Park, Suk
    • Journal of KIISE:Databases
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    • v.29 no.2
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    • pp.119-127
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    • 2002
  • Video server which stores video streams should serve more users with the requested streams rapidly, satisfying their time constraints. However, the number of users supported and the response times for the requested services in video server are in the oppositional relationship with viewpoint of disk throughput. In this paper, we propose new policy that can provide not only rapid responses for the service requests but also increase the number of users supported in the storage system of video server. The policy admits the random movements of disk heads for urgent service requests but maintains the sequential or restricted movements of disk heads and eliminates rewind time of disk heads for less-urgent service requests in storage system of multiple disks environment so that it can not satisfy only the QoS of users but also support more users.

Metadata Management of a SAN-Based Linux Cluster File System (SAN 기반 리눅스 클러스터 파일 시스템을 위한 메타데이터 관리)

  • Kim, Shin-Woo;Park, Sung-Eun;Lee, Yong-Kyu;Kim, Gyoung-Bae;Shin, Bum-Joo
    • The KIPS Transactions:PartA
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    • v.8A no.4
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    • pp.367-374
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    • 2001
  • Recently, LINUX cluster file systems based on the storage area network (SAN) have been developed. In those systems, without using a central file server, multiple clients sharing the whole disk storage through Fibre Channel can freely access disk storage and act as file servers. Accordingly, they can offer advantages such as availability, load balancing, and scalability. In this paper, we describe metadata management schemes designed for a new SAN-based LINUX cluster file system. First, we present a new inode structure which is better than previous ones in disk block access time. Second, a new directory structure which uses extendible hashing is described. Third, we describe a novel scheme to manage free disk blocks, which is suitable for very large file systems. Finally, we present how we handle metadata journaling. Through performance evaluation, we show that our proposed schemes have better performance than previous ones.

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Study of the Tribological Characteristics Based on the Hardness of the Brake Disk between the Sintered Metallic Friction Material and the Heat-resisting Steel Disks (디스크 경도에 따른 소결마찰재와 내열강 디스크의 마찰·마모 특성)

  • Na, Sun Joo;Park, Hyoung Chul;Kim, Sang Ho
    • Tribology and Lubricants
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    • v.31 no.2
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    • pp.42-49
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    • 2015
  • Because of the growing need for high-speed transport options such as trains and aircraft, there is increasing demand for technology related to high-speed trains. Among them, braking systems are important in high-speed trains in terms of reliability. Especially, the disk brake system, in use in most high-speed trains, transforms kinetic energy into thermal energy and noise. Therefore, the material properties of both the friction materials and disks are expected to influence the tribological characteristics. In this paper, the tribological characteristics depend on the hardness of the brake disks between the Cu-based sintered metallic friction material and the heat-treated heat-resisting steel disks. A lab-scale dynamometer used to perform braking tests at a variety of braking speeds using dry conditions. The test results revealed that the hardness of the disks affects the friction coefficients, friction stabilities, and wear rates. Thus, the brake system using the heat-resisting steel disk requires proper heat-treatment. These differences are considered to be caused by the change in tribological mechanisms and the generation of an oxide layer on the friction surfaces. The oxide layers on the friction surfaces are confirmed to Fe2O3 by x-ray diffraction (XRD) and scanning electron microscope-energy dispersive spectroscopy (SEM-EDS) analysis.

Phenotypic and Genotypic Detection of Metallo-β-Lactamase Producing Pseudomonas aeruginosa

  • Yang, Byoung-Seon;Hong, Keun-Seok;Jung, Seung-Bong;Kwon, Young-Hoon;Jeong, Jong-Yoon;Lee, Min-Joo;Lee, Hye-In;Park, Mi-Seon;Choi, Seung-Gu
    • Korean Journal of Clinical Laboratory Science
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    • v.44 no.2
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    • pp.81-85
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    • 2012
  • This study was undertaken to evaluate phenotypic and genotypic methods for detection of Metallo-Beta-Lactamases (MBLs) among nosocomial Pseudomonas aeruginosa. Of the 50 P. aeruginosa isolates from clinical specimens, 20 were evaluated for carbapenem resistance and screened for MBL by double-disk synergy test and combined-disk test. Nineteen strains (95%) were found to be MBL producers among the 20 P. aeruginosa. MBL positives were further confirmed by Polymerase Chain Reaction (PCR). For the IMP and VIM types of MBLs, PCR analysis was performed on 19 of the 20, and 10 were positive for VIM MBL type. This study reports the validation of a simple and accurate MBL detection method that can be easily incorporated into the daily routine of a clinical laboratory. Early detection of MBL-carrying organisms, including those with susceptibility to carbapenems, is of paramount clinical importance, as it allows rapid initiation of strict infection control practices as well as therapeutic guidance for confirmed infection.Key Words : Hepatitis A virus (HAV), Anti-HAV, Hospital workers, Prevalence, Vaccination

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How are S0 galaxies formed? A case of the Sombrero galaxy

  • Kang, Jisu;Lee, Myung Gyoon;Jang, In Sung;Ko, Youkyung;Sohn, Jubee;Hwang, Narae;Park, Byeong-Gon
    • The Bulletin of The Korean Astronomical Society
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    • v.44 no.1
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    • pp.38.2-38.2
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    • 2019
  • S0 galaxies are mostly known to be formed in dense environments from spiral progenitors. Recently, however, a new formation scenario has been suggested that field S0s can be formed from elliptical progenitors. The Sombrero galaxy (M104, NGC 4594) is a massive disk galaxy located in the field environment, and its morphological type has been controversial from Sa to E. Thus, it is an ideal target to test the new scenario. We trace the giant halo of M104 with globular clusters to test this scenario. From the wide images obtained with CFHT/MegaCam, we find a large number of globular clusters in this galaxy. We also confirm their membership by measuring the radial velocities from the spectra obtained with MMT/Hectospec. The color distribution of these globular clusters is bimodal, and blue (metal-poor) globular clusters are more spatially widely spread than red (metal-rich) globular clusters. This indicates that M104 hosts a giant metal-poor halo as well as an inner metal-rich halo. Combining this result with the fact that M104 is unusually massive and brighter than other spiral galaxies, we infer that M104 was indeed a massive elliptical galaxy that had formed a metal-rich halo by gas-rich mergers and a metal-poor halo by gas-poor mergers. In addition, we find young star clusters around the disk of M104, which shows that the disk formed after the spheroidal halos had formed. In conclusion, we suggest that M104 was originally a massive elliptical galaxy and was transformed to a lenticular galaxy by acquiring its disk later.

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Relationship between rotational disc displacement of the temporomandibular joint and the dentoskeletal morphology

  • Park, So-Hyun;Han, Won-Jeong;Chung, Dong-Hwa;An, Jung-Sub;Ahn, Sug-Joon
    • The korean journal of orthodontics
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    • v.51 no.2
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    • pp.105-114
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    • 2021
  • Objective: The purpose of this study was to evaluate the relationship between rotational disk displacement (DD) of the temporomandibular joint (TMJ) and the dentoskeletal morphology. Methods: Women aged > 17 years were included in this study. Each subject had a primary complaint of malocclusion and underwent routine cephalometric examinations. They were divided into five groups according to the findings on sagittal and coronal magnetic resonance images of their TMJs: bilateral normal disk position, bilateral anterior DD with reduction (ADDR), bilateral rotational DD with reduction (RDDR), bilateral anterior DD without reduction (ADDNR), and bilateral rotational DD without reduction (RDDNR). Twenty-three cephalometric variables were analyzed, and the Kruskal-Wallis test was used to evaluate differences in the dentoskeletal morphology among the five groups. Results: Patients with TMJ DD exhibited a hyperdivergent pattern with a retrognathic mandible, unlike those with a normal disk position. These specific skeletal characteristics were more severe in patients exhibiting DD without reduction than in those with reduction, regardless of the presence of rotational DD. Rotational DD significantly influenced horizontal and vertical skeletal patterns only in the stage of DD with reduction, and the mandible exhibited a more backward position and rotation in patients with RDDR than in those with ADDR. However, there were no significant dentoskeletal differences between ADDNR and RDDNR. Conclusions: The results of this study suggest that rotational DD of TMJ plays an important role in the dentoskeletal morphology, particularly in patients showing DD with reduction.

FLAT-FIELDING FOR SOLAR FULL DISK Hα MONITORING SYSTEM OF KASI (한국천문연구원 Hα 태양전면관측시스템의 바닥고르기 연구)

  • Park, H.M.;Kim, Y.H.;Bong, S.C.;Park, Y.D.;Cho, K.S.;Jang, B.H.;Choi, S.;Nah, J.;Lee, S.M.;Chae, J.
    • Publications of The Korean Astronomical Society
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    • v.23 no.2
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    • pp.47-52
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    • 2008
  • We have performed the flat-fielding correction for the $H{\alpha}$ full-disk monitoring system of KASI (Korea Astronomy and Space Science Institute), which is installed in the Solar Flare Telescope (SOFT) at the top of Bohyun Mountain. For this, we used a new method developed by Chae (2004), to determine the flat pattern from a set of relatively shifted images. Using this method, we successfully obtained the flat pattern for $H{\alpha}$ full-disk observations and compared our result with the image observed in Catania Astrophysical Observatory. The method that we used in this study seems to be quite powerful to obtain the flat image for solar observations. In near future, we will apply this method for the flat-fielding correction of all solar imaging instruments in KASI.