• 한국산학기술학회논문지
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• 제3권2호
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• pp.131-135
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• 2002

지하수의 오염을 막기 위하여 음식물의 매립은 법적 제재를 받는다. 따라서 음식물을 퇴비나 사료로 사용할 수 있는 시스템을 갖추는 것이 바람직하다. 이러한 필요에 따라 음식물 쓰레기 처리용 원적외선 가열기를 법랑 및 전열선을 사용하여 설계하였고, 가열의 효과를 돕기 위한 원적외선 발열 교반기도 설계하였다. 또한 물을 많이 포함하고 있는 음식물 쓰레기의 발효에 알맞은 발열체의 온도가 190℃ 부근임과 원적외선 발열체의 인적외선 방사효율을 조사한 결과 흑색의 법랑이 적절함을 확인하였다.

• 천문학회보
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• 제38권2호
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• pp.87.2-87.2
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• 2013

We studied a fine-scale half ring-like structure around a pore seen from the high spectral and the high spatial resolution data. Our observations were carried out using the Fast Imaging Solar Spectrograph (FISS) and the InfraRed Imaging Magnetograph (IRIM) installed at the 1.6 meter New Solar Telescope of Big Bear Solar Observatory (BBSO) on 2012 July 19. During the observations, we found a fine-scale half ring-like structure located very close to a pore (~0.4 arcsec apart from the pore). It was seen in the far wing images of the $H{\alpha}$ and Ca II $8542{\AA}$ lines, but it was not seen in the line center images of two lines. The length of the structure is about 4200 km and the width is about 350 km. We determined its line-of-sight velocity using the Doppler shift of the centroid of the Ti II line ($6559.6{\AA}$, close to the $H{\alpha}$ line) and determined horizontal velocity using the NAVE method. we also investigated the magnetic configurations using the Stokes I, Q, U, and V maps of the IRIM. As a results, we found that it has a high blue-shift velocity (~2km) faster than the photospheric features and has a strong horizontal component of the magnetic field. Based on our findings, we suggest that it is associated with small flux emergence, which occurs very close to the pore. Even though it is very small structure, this kind of magnetic configuration can be in chare of the upper chromosphere heating, especially above the pore.