• 한국조명전기설비학회지:조명전기설비
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• 제9권6호
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• pp.32-40
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• 1995

Far Infrared radiators should have functionality to convert thermal energy into an electromagnetic wave. In order to apply the Far Infrared to the substance, the absorption characteristics of the substance should be considered. In this paper, interrelation of emissivity with emission energy according to temperature in the range of [$2.5\mu\textrm{m}$] to 25[$\mu\textrm{m}$] after the transition element oxides (MnO2, Fe2O3, CuO, Co3O4) of first grade reagent were molded in press, then they were sintered in [$1050^{\circ}C$], and they were used as samples.

• 천문학회지
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• 제40권4호
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• pp.113-118
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• 2007

Recently far infra-red (FIR) polarization of the $850{\mu}m$ continuum emission from T Tauri disks has been detected. The observed degree of polarization is around 3 %. Since thermal emission from dust grains dominates the spectral energy distribution at the FIR regime, dust grains might be the cause of the polarization. We explore alignment of dust grains by radiative torque in T Tauri disks and provide predictions for polarized emission for disks viewed at different wavelengths and viewing angles. In the presence of magnetic field, these aligned grains produce polarized emission in infrared wavelengths. When we take a Mathis-Rumpl-Nordsieck-type distribution with maximum grain size of $500-1000{\mu}m$, the degree of polarization is around 2-3 % level at wavelengths larger than ${\sim}100{\mu}m$. Our study indicates that multifrequency infrared polarimetric studies of protostellar disks can provide good insights into the details of their magnetic structure.

• Journal of Photoscience
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• 제4권3호
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• pp.121-125
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• 1997

The 77 K emission and excitation, and room-temperature visible spectra of cis[Cr(cyclam)Br$_2$]Br (cyclam=1,4,8,11-tetraazacyclotetradecane) are reported. The mid- and far-infrared spectra at room-temperature are also measured. The vibrational intervals of the electronic ground state are extracted from the far-infrared and emission spectra. The ten electronic bands due to spin-allowed and spin-forbidden transitions are assigned. It is found that nitrogen atoms of the cyclam ligand have strong $\sigma$-donor characters, but bromide ligand has weak $\sigma$- and $\pi$-donor properties toward chromium(III) ion. The zerophonon line in the excitation spectrum splits into two components by 172 cm$^{2-}$, and the large $^2E_g$ splitting can be reproduced by the ligand field theory.

• 천문학회보
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• 제36권2호
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• pp.71.1-71.1
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• 2011

Significant discrepancies have been found between the dust masses of edge-on spiral galaxies derived from various tracers (optical/near-infrared, far-infrared/sub-millimeter observations, and the variation of dust attenuation with viewing angle). Here we report the first detection of a vertically extended far-ultraviolet (FUV) and near-UV (NUV) emission in an edge-on spiral galaxy NGC 891. The vertically extended emission is interpreted as the dust-scattered light due to a extraplanar dust layer in NGC 891 that contains about the same mass as the standard thin dust disk. This new dust component completely encloses the stellar disk and bulge, and solves the puzzle of dust mass.

• Bulletin of the Korean Chemical Society
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• 제20권1호
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• pp.81-84
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• 1999

The emission and excitation spectra of [Cr(NH3)5(imH)](ClO4)3·H2O (imH=imidazole) taken at 77 K are reported. The 298 K visible and far-infrared spectra are also measured. The vibrational intervals of the electronic ground state are extracted from the far-infrared and emission spectra. The ten electronic bands due to spin-allowed and spin-forbidden transitions are assigned. Using the observed transitions, a ligand field analysis has been performed to determine the bonding properties of coordinated imidazole in the title chromium(Ⅲ) complex. It is confirmed that nitrogen atom of the imidazole ligand has a medium it-acceptor property toward chromium(Ⅲ) ion. The zero-phonon line in the excitation spectrum splits into two components by 181 cm-1, and the large 2Eg splitting can be reproduced by the ligand field theory.

• 천문학논총
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• 제27권4호
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• pp.161-164
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• 2012

We performed a spectroscopic survey for cometary volatiles with the Infrared Camera onboard the Japanese infrared satellite AKARI. The observations were carried out in the near-infrared wavelength range in the period from 2008 June to 2010 January. In this paper, we summarize the observations and results of the AKARI survey for the mixing ratios of major volatiles in comets. We derived the $2.5-5{\mu}m$ spectra of 18 comets including both Oort cloud comets and Jupiter-family comets. Prominent emission bands in the observed spectra are the fundamental vibrational bands of water ($H_2O$) at $2.7{\mu}m$ and carbon dioxide ($CO_2$) at $4.3{\mu}m$. The fundamental vibrational band of carbon monoxide (CO) at $4.7{\mu}m$ and the broad emission feature probably related to C-H bearing molecules can also be recognized around the $3.4-3.5{\mu}m$ region in some comets. We detect $CO_2$ in 17 out of 18 comets, and derived gas production rate ratios of $CO_2$ with respect to $H_2O$ in 17 comets. We detect a reliable CO emission band only in three of the comets. Our data set provides the largest homogeneous database of $CO_2/H_2O$ ratios in comets obtained so far.

• 천문학논총
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• 제27권4호
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• pp.275-279
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• 2012

We investigate the mid-infrared (MIR) to far-infrared (FIR) properties of a nearly complete sample of local active galactic nuclei (AGNs) detected in the Swift/Burst Alert telescope (BAT) all-sky hard X-ray (14-195 keV) survey, based on the cross correlation with the infrared survey catalogs of AKARI, IRAS and WISE. Out of 135 non-blazar AGNs in the Swift/BAT 9-month catalog, we obtain the MIR photometric data for 128 sources in either the 9, 12, 18, 22, and $25{\mu}m$ band. We find a good correlation between their hard X-ray and MIR luminosities ranging three orders of magnitude (42 < log ${\lambda}L_{\lambda}$(9, $18{\mu}m$) < 45), which is tighter than that with the FIR luminosities at $90{\mu}m$. Both X-ray unabsorbed and absorbed AGNs follow the same correlation, implying isotropic infrared emission, as expected in clumpy dust tori models rather than homogeneous ones.

• 한국가금학회지
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• 제42권2호
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• pp.125-132
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• 2015

원적외선은 자연계의 태양에너지의 한 부분으로 가시광선의 적색영역보다 파장이 월등히 길어서 열작용이 크며, 생체 내 침투력이 강한 파장으로 알려져 있다. 본 연구에서는 육계를 사육하는 과정에서 일정량의 원적외선을 조사하는 방법으로 육계의 건강 증진은 물론, 사육환경의 개선 효과의 가능성을 검정하고자 하였다. 세미브로(Ross ♂ ${\times}$ Hyline ♀) 암수 무감별추 200수를 공시하여 흰색조명, White구(5,000~5,700 K), 흰색조명+원적외선 조사(White+FIR구), 녹색조명, Green구(525~570 nm) 녹색조명+원적외선(Green+FIR구)의 4처리, 처리당 2반복으로 실험을 실시하였다. 전 사육기간 중 증체량과 사료효율은 녹색조명 환경이 백색조명 환경보다 높게 나타나는 경향이 인정되었다. 이러한 증가는 두 조명 모두 원적외선 조사에 의해서 더 증가되는 경향이 인정되었다. 사육장 바닥 깔짚 내 ammonia 및 저급탄화수소의 발생량은 조명의 색깔에 따른 차이는 인정되지 않았지만, 두 조명 모두 원적외선 조사에 의해서 ammonia 및 저급탄화수소의 발생량이 감소하는 경향이 인정되었다. 혈장 내 AST의 농도는 녹색조명 처리구가 백색조명 처리구보다 낮게 나타났으며, 이러한 경향은 두 조명 모두 원적외선의 조사에 의해서 더 감소되어서 백색조명 처리구보다 녹색조명에 원적외선을 조사한 처리구에서 유의하게 낮게 나타났다(P<0.05). 혈액 중 albumin 및 각종 면역 글로블린(LgA, lgG 및 lgM)의 농도는 조명의 차이에 따른 변화는 인정되지 않았지만, 흰색조명, 녹색조명 모두 원적외선 조사에 따라서 증가하는 경향이 나타났다. 결론적으로 육계 사육과정에 원적외선의 조사는 사육환경 개선 및 생리활성물질의 증가에 영향을 미쳐서 생산성을 증가시킬 가능성이 있다고 생각되어진다.

• 천문학논총
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• 제27권4호
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• pp.213-216
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• 2012

We have collected dozens of mid-infrared spectra showing UIR bands from diffuse Galactic emitting regions with the AKARI's Infrared Camera (IRC) onboard AKARI, as part of the ISMGN Mission Program. The datasets cover various directions in the inner Galactic Plane ($|l|$ < 70 deg), in the outer Galactic Plane ($|l|$ > 70 deg), and in the off-Plane ($|b|$ > 2 deg). The variations in the UIR band ratios are examined in terms of the radiation environments judged from the far-infrared ($50-170{\mu}m$) spectral energy distribution (SED) made with AKARI/FIS All Sky Survey data at each slit position where mid-IR spectra were obtained. We have found that the band ratios of $6.2{\mu}m/11.2{\mu}m$ and $7.7{\mu}m/11.2{\mu}m$ toward the inner Galaxy are systematically higher than those toward the outer Galaxy and off the Galactic plane. Likely causes of the variations in properties of UIR bands in diffuse emission on a Galactic scale are discussed in this paper.

• Journal of the Korean Wood Science and Technology
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• 제36권6호
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• pp.113-120
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• 2008

본 연구는 포름알데히드와 같은 유해화학물질을 저감하고, 인체에 무해한 친환경 건축마감재를 개발하기 위하여 대나무숯분말, 편백추출수 및 바인더를 원료로 이용하여 실내 건축마감재용 액상코팅제를 제조하였다. 편백추출수의 함유량에 따른 액상코팅제의 유해화학물질에 대한 탈취율, 원적외선방사율, 음이온방출량, 항균성 및 실제 소요량을 조사하였다. 액상코팅제의 포름알데히드 탈취율은 60.0~98.6%, 암모니아 탈취율은 76.7~86.2%였다. 편백추출수의 혼합량이 증가함에 따라 탈취율도 증가하는 경향을 보였다. 액상코팅제의 원적외선방사율은 91.7%, 음이온 방출량은 77개/cc 였으며, 세균감소율은 99.4%로 항균력이 우수하였으나, 편백추출수의 혼합량 증가에 따른 이들 값에는 차이가 인정되지 않았다. 액상코팅제의 소요량은 스프레이건을 사용할 경우 $0.66kg/m^2$, 붓칠의 경우 $0.94kg/m^2$로 스프레이건을 이용할 경우가 더 효율적이었다.