• Title/Summary/Keyword: Far infra red heating

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Physical Approach of the FIR Heater Design for Food Waste Fermentation (음식물 쓰레기 발효기 제작을 위한 원적외선 가열장치 설계의 물리학적 접근)

  • 한두희
    • Journal of the Korea Academia-Industrial cooperation Society
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    • v.3 no.2
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    • pp.131-135
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    • 2002
  • The reclamation of food waste is brought by law in order to clean the underground water. Thus the food waste feed back system should be prepared. The electric heater and mixing tool for FIR radiation were developed in order to control the food waste fermentation. Also we suggest the optimum temperature 19$0^{\circ}C$, black enamel ware for food waste control.

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A Fine-scale Half Ring-like Structure around a Pore

  • Song, Donguk;Chae, Jongchul
    • The Bulletin of The Korean Astronomical Society
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    • v.38 no.2
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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.

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