• 한국전기전자재료학회:학술대회논문집
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• 한국전기전자재료학회 2006년도 하계학술대회 논문집 Vol.7
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• pp.249-250
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• 2006

Bi-2212/Ag ROSAT용 와이어의 제작은 PIT법으로 제작된 단일 필라멘트가 사용되었다. 제작된 필라멘트를 압연하여 너비 8.6mm, 두께 2.15mm의 압연 테입을 제조한 후 4개씩 적층하여 3 부분의 마름모로 만들어 다시 내경 17.2mm의 Ag튜브에 적층하여 ROSAT 와이어를 약 150 mm로 제작하였다. 제작된 ROSAT 와이어는 산소분위기에서 약 60시간 동안 열처리 되었다. 이때 열처리 온도와 최고점에서의 유지시간에 따른 Bi-2212/Ag ROSAT 와이어의 전기적 특성을 평가 하였다. 기존의 Bi-2212/Ag 와이어에 비해 압연, 적층, 인발하여 제작된 동일한 크기의 ROSAT 와이어가 향상된 전기적 특성을 나타내었다.

• Progress in Superconductivity
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• 제9권1호
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• pp.111-114
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• 2007

We have investigated the effect of different heat treatment processes on electrical and magnetic properties of Bi2212/Ag ROSAT wire. The ROSAT wire was fabricated by stacking and arranging 12 filaments Bi2212/Ag tapes in triple rotation symmetry in a Ag tube. ROSAT wires have been prepared using a partial melting method with changing $T_{max}$ and $T_a$ in oxygen atmosphere. The highest critical current density($J_c$) at 65 K under 0 T was $21,158\;A/cm^2$ for wire prepared $890\;^{\circ}C(T_{max})$ and $840\;^{\circ}C(T_a)$, respectively. SEM results indicated that the wire prepared at $890\;^{\circ}C(T_{max})$ and $840\;^{\circ}C(T_a)$ showed better directional phases than the other samples. However the result of magnetic susceptibility measurement indicates that the wire prepared $890\;^{\circ}C(T_{max})$ and $835\;^{\circ}C(T_a)$ had better superconducting phases than the other samples. It was revealed that heat treatment temperature was important factor for superconducting properties of the ROSAT wire.

• 한국초전도학회:학술대회논문집
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• 한국초전도학회 2006년도 High Temperature Superconductivity Vol.XVI
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• pp.93-93
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• 2006

• 한국초전도학회:학술대회논문집
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• 한국초전도학회 2007년도 High Temperature Superconductivity Vol.XVII
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• pp.73-73
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• 2007

• 천문학논총
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• 제8권1호
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• pp.199-206
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• 1993

We review recent systematic investigation of the X-ray spectra of early type galaxies by using the Einstein data base and present new results by the ROSAT observations. The Einstein data suggested that the galaxies with low X-ray to optical luminosity ratio may have another very soft component. ROSAT observations confirm its presence and call for further study to understand the nature of this very soft emission. The X-ray bright galaxies have emission temperature of ${\sim}\;0.8\;keV$ and show radial gradients in the sense that X-ray emission is softer and more absorbed in the inner region.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 1996년도 한국우주과학회보 제5권2호
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• pp.38-46
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• 1996

• 천문학회보
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• 제18권
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• pp.12.2-12.2
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• 1993

• 천문학회보
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• 제17권
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• pp.19.2-19.2
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• 1992

• 천문학회지
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• 제38권1호
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• pp.1-6
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• 2005

We searched for X-ray emission from the 665 galaxies inside and towards the nearby voids by analyzing the ROSAT All-Sky Survey (RASS) data as well as the ROSAT pointed observations (PSPC). As a result we have detected six X-ray emitting galaxies. Two (UGC 10205 and NGC 7509) are in the high density region in the local void, three (UGC 749, MCG +11-10-073, and Mrk 464) are towards the nearby voids, and UGC 32 is located in the low density region. We carried out a timing analysis for both Mrk 464 and UGC 32, and a spectral analysis for Mrk 464. The light curve of Mrk 464 shows the possibility of periodic X-ray flux variation and UGC 32 shows weak, but rapid variation.

• 천문학회보
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• 제20권
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• pp.5.2-5.2
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• 1995