• 천문학회지
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• 제50권6호
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• pp.167-178
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• 2017

We present a study of the inexplicit connection between radio jet activity and ${\gamma}$-ray emission of BL Lacertae (BL Lac; 2200+420). We analyze the long-term millimeter activity of BL Lac via interferometric observations with the Korean VLBI Network (KVN) obtained at 22, 43, 86, and 129 GHz simultaneously over three years (from January 2013 to March 2016); during this time, two ${\gamma}$-ray outbursts (in November 2013 and March 2015) can be seen in ${\gamma}$-ray light curves obtained from Fermi observations. The KVN radio core is optically thick at least up to 86 GHz; there is indication that it might be optically thin at higher frequencies. To first order, the radio light curves decay exponentially over the time span covered by our observations, with decay timescales of $411{\pm}85$ days, $352{\pm}79$ days, $310{\pm}57$ days, and $283{\pm}55$ days at 22, 43, 86, and 129 GHz, respectively. Assuming synchrotron cooling, a cooling time of around one year is consistent with magnetic field strengths $B{\sim}2{\mu}T$ and electron Lorentz factors ${\gamma}$ ~ 10 000. Taking into account that our formal measurement errors include intrinsic variability and thus over-estimate the statistical uncertainties, we find that the decay timescale ${\tau}$ scales with frequency ${\nu}$ like ${\tau}{\propto}{\nu}^{-0.2}$. This relation is much shallower than the one expected from opacity effects (core shift), but in agreement with the (sub-)mm radio core being a standing recollimation shock. We do not find convincing radio flux counterparts to the ${\gamma}$-ray outbursts. The spectral evolution is consistent with the 'generalized shock model' of Valtaoja et al. (1992). A temporary increase in the core opacity and the emergence of a knot around the time of the second ${\gamma}$-ray event indicate that this ${\gamma}$-ray outburst might be an 'orphan' flare powered by the 'ring of fire' mechanism.

• 대한방사선기술학회지:방사선기술과학
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• 제44권4호
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• pp.359-365
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• 2021

A heavy particle accelerator is a device that accelerates particles using high energy and is used in various fields such as medical and industrial fields as well as research. However, secondary neutrons and particle fragments are generated by the high-energy particle beam, and among them, the neutrons do not have an electric charge and directly interact with the nucleus to cause radiation of the material. Quantitative evaluation of the radioactive material produced in this way is necessary, but there are many difficulties in actual measurement during or after operation. Therefore, this study compared and evaluated the generated radioactive material in the concrete shield for protons and carbon ions of specific energy by using the simulation code FLUKA. For the evaluation of each energy of proton beam and carbon ion, the reliability of the source term was secured within 2% of the relative error with the data of the NASA Space Radiation Laboratory(NSRL), which is an internationally standardized data. In the evaluation, carbon ions exhibited higher neutron flux than protons. Afterwards, in the evaluation of radioactive materials under actual operating conditions for disposal, a large amount of short-lived beta-decay nuclides occurred immediately after the operation was terminated, and in the case of protons with a high beam speed, more radioactive products were generated than carbon ions. At this time, radionuclides of ⁴⁴Sc, ³H and ²²Na were observed at a high rate. In addition, as the cooling time elapsed, the ratio of long-lived nuclides increased. For nonparticulate radionuclides, ³H, ²²Na, and for particulate radionuclides, ⁴⁴Ti, ⁵⁵Fe, ⁶⁰Co, ¹⁵²Eu, and ¹⁵⁴Eu nuclides showed a high ratio. In this study, it is judged that it is possible to use the particle accelerator as basic data for facility maintenance, repair and dismantling through the prediction of radioactive materials in concrete according to the cooling time after operation and termination of operation.

• 한국농림기상학회지
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• 제22권4호
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• pp.327-339
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• 2020

증산은 물이 기공을 통해 대기 중으로 이동하는 과정으로, 지표면의 물은 상당부분 증산을 통해 대기 중으로 이동한다. 에디공분산, 수분 수지 측정법 등의 증산량을 측정하는 방법이 있지만, 수종 및 임분의 구성 요소별 증산량의 차이를 비교하기 위해서는 개체목 증산량 측정이 필요하다. 개체목 증산량을 측정하기 위해 수액의 온도차를 이용한 수액류 측정법을 가장 널리 이용하고 있지만, 넓은 범위의 지역을 장기간 조사하기에 한계가 있다. 따라서 큰 공간적 규모에 대해 수액류 및 증산량에 대한 연구를 하기 위해서는 각 지역별로 측정한 데이터의 공유가 필요하다. 본 연구팀은 태화산 학술림에서 열손실탐침법을 이용하여 2011년부터 잣나무(Pinus koraiensis) 18본, 2013년부터 갈참나무(Quercus aliena) 16본을 대상으로 수액류를 측정하고 있으며, 광릉수목원에서도 열손실탐침법을 이용하여, 2013년부터 전나무(Abies holophylla) 18본, 졸참나무(Quercus serrata) 7본, 서어나무(Carpinus laxiflora) 3본, 까치박달(Carpinus cordata) 3본을 대상으로 수액류를 측정하고 있다. 구례 지리산 조사지에서는 열 파동법으로 2018년부터 산벚나무(Prunus sargentii), 낙엽송(Larix kaempferii), 2019년에는 추가로 상수리나무(Quercus accutisima), 소나무(Pinus densiflora), 물푸레나무(Fraxinus rhynchophylla)를 대상으로 수액류를 측정하였으며, 2020년에는 편백(Chamecypans obtuse), 잣나무(P. koraiensis), 자작나무(Betulla platyphylla), 전나무(A. holophylla), 곰솔(Pinus thrunbergii)을 대상으로 수액류를 측정하고 있다. 우리나라 산림의 수액류 데이터를 더욱 활발하게 공유하여 국내 산림생태계에서 개체목과 임분의 수액류와 증산의 환경민감성 등 다양한 연구에 기여할 것으로 기대한다.