• Title/Summary/Keyword: Spiral imaging

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CO and HI Properties of the Virgo Cluster Spiral Galaxies

  • Chung, Eun-Jung;Rhee, Myung-Hyun;Kim, Hyo-Ryoung;Chung, Ae-Ree;Yun, Min-S.
    • Bulletin of the Korean Space Science Society
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    • 2009.10a
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    • pp.36.1-36.1
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    • 2009
  • We investigate the molecular and atomic gas properties of 20 Virgo cluster spiral galaxies by comparing with optical properties to assess the effect of the Virgo environment on the interstellar media of the Virgo disks. CO maps from FCRAO On-The-Fly (OTF) mapping survey and HI maps from VIVA (VLA Imaging of Virgo spirals in Atomic gas) are shown, and radial properties of molecular and atomic gas are compared. H2 deficiency along with HI is investigated, and gas evolution history of the Virgo cluster spirals is also examined.

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Off-resonance Correction by Autofocus algorithm for Spiral Scan Imaging at 3Tesla MRI (자동초점 조절 방식을 통한 나선주사 영상의 off-resonance 보정 알고리즘)

  • Kang, Seung-Won;Kim, Pan-Ki;Cho, Sang-Heum;Ahn, Chang-Beom
    • Proceedings of the KIEE Conference
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    • 2007.07a
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    • pp.1920-1921
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    • 2007
  • 본 논문에서는 나선주사 영상에서 발생하는 off-resonance 현상에 의한 영상의 번짐을 보정하는 새로운 알고리즘을 제안하였다. 공간상에서의 inhomogeneity와 chemical-shift 현상으로 생기는 off-resonance 효과는 공간의 자장의 세기에 비례한다. 현재 사용되고 있는 보정 방법에서의 절차를 간소화 하고 보다 효과적인 보정 알고리즘을 적용함으로써 보다 나은 Spiral scan 영상을 얻고자 하였다.

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Lung Perfusion Imaging and $Tc^{99m}-Macroaggregated$ Human Serum Albumin

  • Haider, Kh.H.;Ilyas, M.;Hyder, Q.;Kim, Chong-Kook
    • Journal of Pharmaceutical Investigation
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    • v.31 no.2
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    • pp.73-80
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    • 2001
  • Lung perfusion scanning, invariably combined with ventilation studies provides a reliable and non-invasive mean to diagnose lung related pathologies despite the availability of modern techniques such as angiography, magnetic resonance imaging, magnetic resonance angiography, and helical (spiral) computed tomography. The technique involves the generation of images by radiations emitted from radioisotopes introduced in to the lungs. Various radiopharmaceuticals have been proposed and designed to incorporate $Tc^{99m}$ in to macroparticulate form for lung perfusion imaging. However, most of these have associated difficulties such as reproducibility of the product with regards to particle size distribution and poor elimination from the lung capillary bed. $Tc^{99m}$ macroaggregated albumin $(Tc^{99m}-MAA)$ is used extensively for clinical lung perfusion imaging and is considered as the radiopharmaceutical of choice. It is non-toxic, safe, and being biodegradable, is easily eliminated from the lung capillary bed by proteolytic enzyme metabolism and by mechanical forces due to lung movement.

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Small (2 cm) Hepatic Lesions in Colorectal Cancer Patients: Detection and Characterization on Mangafodipir Trisodium-enhanced MR Imaging

  • 김경원;김아영;박성호;김현진;박미숙;김태경;하현권;김표년;이문규
    • Proceedings of the KSMRM Conference
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    • 2003.10a
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    • pp.41-41
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    • 2003
  • To evaluate whether mangafodipir trisodium (Mn-DPDP)-enhanced magnetic resonance (MR) imagingimproves the detection and characterization of small (2 cm) hepatic lesions in patients with colorectal carcinoma, compared with spiral CT.

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Patient radiation dose and protection from cone-beam computed tomography

  • Li, Gang
    • Imaging Science in Dentistry
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    • v.43 no.2
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    • pp.63-69
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    • 2013
  • After over one decade development, cone beam computed tomography (CBCT) has been widely accepted for clinical application in almost every field of dentistry. Meanwhile, the radiation dose of CBCT to patient has also caused broad concern. According to the literature, the effective radiation doses of CBCTs in nowadays market fall into a considerably wide range that is from $19{\mu}Sv$ to $1073{\mu}Sv$ and closely related to the imaging detector, field of view, and voxel sizes used for scanning. To deeply understand the potential risk from CBCT, this report also reviewed the effective doses from literatures on intra-oral radiograph, panoramic radiograph, lateral and posteroanterior cephalometric radiograph, multi-slice CT, and so on. The protection effect of thyroid collar and leaded glasses were also reviewed.

Intraductal ultrasonography for biliary strictures

  • Young Koog Cheon
    • Clinical Endoscopy
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    • v.56 no.2
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    • pp.164-168
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    • 2023
  • When diagnosing the nature of biliary strictures, it is sometimes difficult to perform non-invasive methods such as ultrasound, spiral computed imaging, magnetic resonance imaging, or endoscopic ultrasonography. Thus, treatment decisions are usually based on biopsy results. However, brush cytology or biopsy, which is widely used for biliary stenosis, has limitations owing to its low sensitivity and negative predictive value for malignancy. Currently, the most accurate method is bile duct tissue biopsy under direct cholangioscopy. On the other hand, intraductal ultrasonography administered under the guidance of a guidewire has the advantages of easy administration and being less invasive, allowing for adequate examination of the biliary tract and surrounding organs. This review discusses the usefulness and drawbacks of intraductal ultrasonography for biliary strictures.

PATIAL DISTRIBUTION OF STAR FORMATION ACTIVITY ON NGC 253 BY FIR AND RADIO EMISSION LINES

  • Takahashi, H.;Matsuo, H.;Nakanishi, K.
    • Publications of The Korean Astronomical Society
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    • v.27 no.4
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    • pp.261-262
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    • 2012
  • The aim of this research is to reveal the spatial distribution of the star formation activity of nearby galaxies by comparing CO molecular emission lines with the large area observation in far-infrared (FIR) lines. We report the imaging observations of NGC 253 by FIR forbidden lines via FIS-FTS and CO molecular lines from low to high excitation levels with ASTE, which are good tracers of star forming regions or photo-dissociation regions, especially spiral galaxies, in order to derive the information of the physical conditions of the ambient interstellar radiation fields. The combination of spatially resolved FIR and sub-mm data leads to the star formation efficiency within galaxy. The ratio between the FIR luminosity and molecular gas mass, $L_{FIR}/M_{H_2}$, is expected to be proportional to the number of stars formed in the galaxy per unit molecular gas mass and time. Moreover the FIR line ux shows current star formation activity directly. Furthermore these can be systematic and statistical data for star formation history and evolution of spiral galaxies.

Three dimensional CT analysis of facial asymmetry (안면비대칭 3차원 CT 분석)

  • Yoon, Suk-Ja;Lim, Hoi-Jeong;Kang, Byung-Cheol;Hwang, Hyeon-Shik
    • Imaging Science in Dentistry
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    • v.37 no.1
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    • pp.45-51
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    • 2007
  • Purpose : This study aimed to identify the range of normal facial asymmetry using three-dimensional CT and to develop a simple method of diagnosis of facial asymmetry. Materials and Methods : Twenty eight adults with normal occlusion (16 males and 12 females; mean age 24 years and 1 month) were selected whose faces were assessed to be symmetric by an orthodontist. Three-dimensional reconstructions were obtained utilizing spiral CT scans and an oral and maxillofacial radiologist evaluated nineteen anatomic landmarks in three-dimensional coordinates. Facial asymmetry index of each landmark was caluculated. Results : The range of normal facial asymmetry of each landmark was identified using mean and standard deviation of facial asymmetry index. Conclusions : The range of normal facial asymmetry identified in this study may be used as a diagnostic standard for facial asymmetry analysis.

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An Ultraviolet to Infrared Photometric Study of Star Clusters in the Circumnuclear Star-forming Region of Barred Spiral Galaxy NGC 1672

  • Jang, In-Sung;Lee, Myung-Gyoon
    • The Bulletin of The Korean Astronomical Society
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    • v.36 no.2
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    • pp.78.1-78.1
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    • 2011
  • We report on a photometric study of star clusters in the circumnuclear star-forming region of nearby barred spiral galaxy NGC 1672. We use FUV to NIR imaging data (FUV, U, B, V, R, $H{\alpha}$, I, and H) in the Hubble Space Telescope (HST) archive. We have selected 89 star clusters with V<21.8 (MV<-9) mag in the central 600 pc region, and have derived their age & mass by comparing their colors with theoretical population synthesis models. Most of the star clusters are mildly reddened (E(B-V)~0.2 on average), but some star clusters suffer from severe reddening (E(B-V)>0.6). The mass of the star clusters are in the range from $10^4\;M_{\odot}$ to $10^7\;M_{\odot}$. About half of them are more massive than $10^5\;M_{\odot}$. Their ages range from 1 Myr to several 100 Myr, and concentrate at ~6 Myr and ~40 Myr. It indicates that the episodic starburst in the circumnuclear star-forming region lasted at least several 100 Myr. We find no obvious azimuthal age gradient, but we find a radial age gradient in some regions. We discuss these properties with theoretical expectations.

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