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박희석,오재철 弘益大學校 科學技術硏究所 1998 科學技術硏究論文集 Vol.9 No.2
The primary objective of this research was to establish and quantify the relationship between the physical degradation factors of multimedia telecommunications (teleconferencing) system and subjective human perception. A prototype teleconferencing simulator was developed in two separate sound-chambers equipped with audio/video equipment running under a custom-developed software program. Simulation experiments using the semantic differential methodology were performed utilizing 26 paid participants (14 college students and 12 housewives). The results indicated that audio/video synchronization and the frame rate are the main system factors for both subject groups, but different pattern of factors´influence was found according to the group, implying that the system configuration would hopefully accommodate the characteristics of the end users. Also, a single quality index, developed for system preference, was revealed to be highly correlated with user satisfaction. The results provide some fundamental data on the human subjective perception of multimedia telecommunications quality, and further can help establish the quality standards to enhance service level.
IGRINS NEAR-IR HIGH-RESOLUTION SPECTROSCOPY OF MULTIPLE JETS AROUND LkH<i>α</i>234
Oh, Heeyoung,Pyo, Tae-Soo,Yuk, In-Soo,Park, Byeong-Gon,Park, Chan,Chun, Moo-Young,Pak, Soojong,Kim, Kang-Min,Oh, Jae Sok,Jeong, Ueejeong,Yu, Young Sam,Lee, Jae-Joon,Kim, Hwihyun,Hwang, Narae,Kaplan, K American Astronomical Society 2016 The Astrophysical journal Vol.817 No.2
<P>We present the results of high-resolution near-IR spectroscopy toward the multiple outflows around the Herbig Be star LkH alpha 234 using the Immersion Grating Infrared Spectrograph. Previous studies indicate that the region around LkHa 234 is complex, with several embedded young stellar objects and the outflows associated with them. In simultaneous H- and K-band spectra from HH 167, we detected 5 [Fe II] and 14 H-2 emission lines. We revealed a new [Fe II] jet driven by radio continuum source VLA 3B. Position-velocity diagrams of the H-2 1-0 S(1) lambda 2.122 mu m line show multiple velocity peaks. The kinematics may be explained by a geometrical bow shock model. We detected a component of H-2 emission at the systemic velocity (V-LSR = -10.2 km s(-1)) along the whole slit in all slit positions, which may arise from the ambient photodissociation region. Low-velocity gas dominates the molecular hydrogen emission from knots A and B in HH 167, which is close to the systemic velocity; [Fe II] emission lines are detected farther from the systemic velocity, at V-LSR = -100--130 km s(-1). We infer that the H-2 emission arises from shocked gas entrained by a high-velocity outflow. Population diagrams of H-2 lines imply that the gas is thermalized at a temperature of 2500-3000 K and the emission results from shock excitation.</P>
Detector Mount Design for IGRINS
Jae Sok Oh,Chan Park,Sang-Mok Cha,In-Soo Yuk,Kwijong Park,Kang-Min Kim,Moo-Young Chun,Kyeongyeon Ko,Heeyoung Oh,Ueejeong Jeong,Jakyoung Nah,Hanshin Lee,Daniel T. Jaffe 한국우주과학회 2014 Journal of Astronomy and Space Sciences Vol.31 No.2
The Immersion Grating Infrared Spectrometer (IGRINS) is a near-infrared wide-band high-resolution spectrograph jointly developed by the Korea Astronomy and Space Science Institute and the University of Texas at Austin. IGRINS employs three HAWAII-2RG Focal Plane Array (H2RG FPA) detectors. We present the design and fabrication of the detector mount for the H2RG detector. The detector mount consists of a detector housing, an ASIC housing, a Field Flattener Lens (FFL) mount, and a support base frame. The detector and the ASIC housing should be kept at 65 K and the support base frame at 130 K. Therefore they are thermally isolated by the support made of GFRP material. The detector mount is designed so that it has features of fine adjusting the position of the detector surface in the optical axis and of fine adjusting yaw and pitch angles in order to utilize as an optical system alignment compensator. We optimized the structural stability and thermal characteristics of the mount design using computer-aided 3D modeling and finite element analysis. Based on the structural and thermal analysis, the designed detector mount meets an optical stability tolerance and system thermal requirements. Actual detector mount fabricated based on the design has been installed into the IGRINS cryostat and successfully passed a vacuum test and a cold test.
Detector Mount Design for IGRINS
Oh, Jae Sok,Park, Chan,Cha, Sang-Mok,Yuk, In-Soo,Park, Kwijong,Kim, Kang-Min,Chun, Moo-Young,Ko, Kyeongyeon,Oh, Heeyoung,Jeong, Ueejeong,Nah, Jakyoung,Lee, Hanshin,Jaffe, Daniel T. The Korean Space Science Society 2014 Journal of Astronomy and Space Sciences Vol.31 No.2
The Immersion Grating Infrared Spectrometer (IGRINS) is a near-infrared wide-band high-resolution spectrograph jointly developed by the Korea Astronomy and Space Science Institute and the University of Texas at Austin. IGRINS employs three HAWAII-2RG Focal Plane Array (H2RG FPA) detectors. We present the design and fabrication of the detector mount for the H2RG detector. The detector mount consists of a detector housing, an ASIC housing, a Field Flattener Lens (FFL) mount, and a support base frame. The detector and the ASIC housing should be kept at 65 K and the support base frame at 130 K. Therefore they are thermally isolated by the support made of GFRP material. The detector mount is designed so that it has features of fine adjusting the position of the detector surface in the optical axis and of fine adjusting yaw and pitch angles in order to utilize as an optical system alignment compensator. We optimized the structural stability and thermal characteristics of the mount design using computer-aided 3D modeling and finite element analysis. Based on the structural and thermal analysis, the designed detector mount meets an optical stability tolerance and system thermal requirements. Actual detector mount fabricated based on the design has been installed into the IGRINS cryostat and successfully passed a vacuum test and a cold test.