• The Bulletin of The Korean Astronomical Society
• /
• v.43 no.2
• /
• pp.42.2-43
• /
• 2018

When galaxy clusters interact, the intergalactic gas collides, forming shocks that are characterized by a low sonic Mach number (~3) but a comparatively high Alfvenic Mach number (~30). Such shocks behave differently from the more common astrophysical shocks, which tend to have higher sonic Mach numbers. We wish to determine whether these shocks, despite their low sonic Mach number, are capable of accelerating particles and thereby contributing to the cosmic ray spectrum. Using the PIC-MHD method, which separates the gas into a thermal and a non-thermal component to increase computational efficiency, and relying on existing PIC simulations to determine the rate at which non-thermal particles are injected in the shock, we investigate the evolution of galaxy cluster shocks and their ability to accelerate particles. Depending on the chosen injection fraction of non-thermal particles into the shock, we find that even low-Mach shocks are capable of accelerating particles. However, the interaction between supra-thermal particles and the local magnetic field triggers instabilities and turbulence in the magnetic field. This causes the shock to weaken, which in turn reduces the effectiveness of the supra-thermal particle injection. We investigate how this influences the shock evolution by reducing the particle injection rate and energy and find that a reduction of the particle injection fraction at this stage causes an immediate reduction of both upstream and downstream instabilities. This inhibits particle acceleration. Over time, as the instabilities fade, the shock surface straightens, allowing the shock to recover. Eventually, we would expect this to increase the efficiency of the particle injection and acceleration to previous levels, starting the same series of events in an ongoing cycle of increasing and decreasing particle acceleration.

• Journal of Animal Science and Technology
• /
• v.66 no.1
• /
• pp.31-56
• /
• 2024

Pig farming, a vital industry, necessitates proactive measures for early disease detection and crush symptom monitoring to ensure optimum pig health and safety. This review explores advanced thermal sensing technologies and computer vision-based thermal imaging techniques employed for pig disease and piglet crush symptom monitoring on pig farms. Infrared thermography (IRT) is a non-invasive and efficient technology for measuring pig body temperature, providing advantages such as non-destructive, long-distance, and high-sensitivity measurements. Unlike traditional methods, IRT offers a quick and labor-saving approach to acquiring physiological data impacted by environmental temperature, crucial for understanding pig body physiology and metabolism. IRT aids in early disease detection, respiratory health monitoring, and evaluating vaccination effectiveness. Challenges include body surface emissivity variations affecting measurement accuracy. Thermal imaging and deep learning algorithms are used for pig behavior recognition, with the dorsal plane effective for stress detection. Remote health monitoring through thermal imaging, deep learning, and wearable devices facilitates non-invasive assessment of pig health, minimizing medication use. Integration of advanced sensors, thermal imaging, and deep learning shows potential for disease detection and improvement in pig farming, but challenges and ethical considerations must be addressed for successful implementation. This review summarizes the state-of-the-art technologies used in the pig farming industry, including computer vision algorithms such as object detection, image segmentation, and deep learning techniques. It also discusses the benefits and limitations of IRT technology, providing an overview of the current research field. This study provides valuable insights for researchers and farmers regarding IRT application in pig production, highlighting notable approaches and the latest research findings in this field.

• 한국신재생에너지학회:학술대회논문집
• /
• 2011.05a
• /
• pp.121.1-121.1
• /
• 2011

현재 상용화되고 있는 단결정 실리콘 태양전지는 알루미늄 페이스트를 이용하여 후면의 전 영역에 전계를 형성한다. 최근에는 고효율을 얻기 위하여 후면에 패시베이션 효과와 장파장에 대한 반사도를 증가 시키는 SiNx막을 증착 후, 국부적으로 전계를 형성하는 국부 후면 전극(Local back surface field)기술이 연구되고 있다. 본 연구에서는 전면만 텍스쳐 된 단결정 실리콘 웨이퍼를 이용하였다. Plasma Enhanced Chemical Vapor Deposition(PECVD)를 이용하여 전,후면에 SiNx를 증착 하였고 후면의 국부적인 전극 패턴 형성을 위하여 SiNx 식각용 페이스트를 사용한 스크린 프린팅 기술을 이용하였다. 스크린 프린팅을 이용하여 패턴이 형성된 후면에 알루미늄을 인쇄 한 후 Rapid Thermal Process(RTP)를 이용하여 소성 공정 조건을 변화시켰다. 소성 조건 동안 형성되는 후면 전계층은 peak 온도와 승온속도, 냉각 속도에 따라 형상이나 특성이 변화하기 때문에 소성 조건을 변화시키며 국부적 후면 전계 형성의 최적화에 관한 연구를 수행하였다. 패이스트를 이용하여 SiNx를 식각 후 광학 현미경(Optical Microscopy)을 사용하여 SiNx의 식각 유무를 살펴보았고, RTP로 형성된 국부 전계층의 형성 두께, 주변 부분의 형상을 살피기 위해 도핑 영역을 혼합수용액으로 식각하여 주사 전자 현미경(SEM)을 이용하여 관찰 하였다. 또한 후면의 특성을 살펴보기 위해 분광 광도계(UV/VIS/NIR Spectrophotometer)를 사용하여 후면 SiNx층의 유무에 따른 반사도를 비교, 측정 하였다.

• Journal of Energy Engineering
• /
• v.7 no.1
• /
• pp.113-121
• /
• 1998

In natural convection flows, the fluid velocities are highly dependent on the thermal field and property variations can have a strong effect on both the flow and thermal fields. To examine the effect of property variations, at first, numerical analyses covering wide range of the Prandtl number under the same Rayleigh numbers have been carried out. Next, we have modeled the viscosity and thermal conductivity as parabolic functions of temperature and a comprehensive set of numerical solutions have been obtained to understand the effect. The Prandtl number dependence of Nusselt number is fairly strong even though the effect is still weak compared to the Rayleigh number dependence. When thermophysical properties are dependent on temperature, the flow field showed a fairly weak variation except near boundaries, whereas the temperature field is strongly affected, especially by the temperature dependent thermal conductivity.

• Journal of the Korean Magnetics Society
• /
• v.23 no.1
• /
• pp.26-30
• /
• 2013

This article is experimentally to investigate thermal-flow characteristics of the magnetic fluid for concentric annuli under externally fixed magnetic fields using visualization technique. Temperatures of the inner tube and outer tube in the tested concentric annuli were constantly maintained at both $30^{\circ}C$ and $25^{\circ}C$ and the middle tube was filled with the magnetic fluid. Magnetic field was uniformly applied using 4 permanent magnets at 4 directions of the concentric annuli. As a result, the thermal-flow characteristics of the magnetic fluid for concentric annuli could be controlled by directions of the external magnetic fields.

• The Transactions of the Korean Institute of Electrical Engineers B
• /
• v.51 no.9
• /
• pp.522-529
• /
• 2002

In this paper, computer simulations of the physical Phenomena occurring in the arc region before and after current zero were carried out to evaluate the thermal recovery characteristics of a Laval nozzle. A commercial CFD program "PHOENICS" is used for the simulation and the user-coded subroutines to consider the arcing phenomena were added to this program by the authors. The computed results were verified by the comparison with the test results presented by the research group of GE Co.(General Electric Company). In order to investigate the state of the arc region after current zero, the simulation was carried out with three steps. They are steady state arc simulation, transient arc simulation before current zero, and transient hot-gas flow simulation after current zero. The semi-experimental arc radiation model is adapted to consider the radiation energy transport and Prandtl's mixing length model is employed as the turbulence model. The electric field and the magnetic field were calculated with the same grid structure used for the simulation of the flow field. The post-arc current was calculated to evaluate the thermal recovery characteristics after current zero. Compared with the results obtained by GE Co., it has been found that the critical RRRV(ratio of rise of recovery voltage) will be determined previously by this study.his study.

• Journal of Korean Society on Water Environment
• /
• v.40 no.5
• /
• pp.215-228
• /
• 2024

Lakes are one of major sources of methane gas due to anaerobic decomposition of organic matter in sediments. Since methane released from lakes is a greenhouse gas, it is necessary to investigate factors affecting methane production of lakes. This study conducted field and incubation experiments in Lake Asan in August and October to determine effects of thermal stratification and sediment organic matter characteristics on methane production. Field experiments measured temperature and dissolved oxygen to determine the formation of thermal stratification of lakes. Methane and organic matter characteristics were analyzed using gas chromatography, Total Organic Carbon (TOC) analyzers, and fluorescence spectroscopy. Incubation experiments under anaerobic conditions used sediment and water samples from the same site. Field results showed higher methane fluxes in August and increased Dissolved Organic Carbon (DOC) concentration closer to Asan Bay seawall. Elevated methane fluxes and DOC concentration resulted from intensified anaerobic decomposition formed by thermal stratification. Incubation results indicated that sediment organic matter characteristics influenced methane flux between sites. Statistical analysis revealed that thermal stratification could be a primary factor affecting methane production of lakes. Characteristics of sediment organic matter with respect to quantity and quality could be factors influencing methane production of lakes. Results of this study can serve as fundamental data for predicting methane emissions from lakes due to climate change and for mitigating lake's contributions to global warming.

• Journal of Electrical Engineering and Technology
• /
• v.3 no.1
• /
• pp.121-124
• /
• 2008

This paper presents the fabrication and field emission of carbon nanotube field emitters for a micro mass spectrometer. The carbon nanotube is an adequate material as a field emitter since it has good characteristics. We have successfully fabricated a diode field emitter and a triode field emitter. Each field emitter has been constructed using several micromachining processes and a thermal CVD process. In the case of the diode field emitter, to increase the electric field, the carbon nanotubes are selectively grown on the patterned nickel catalyst layer. The electron current of the diode field emitter is 73.2 ${\mu}A$ when the anode voltage is 1100V. That of the triode field emitter is 3.4 pA when the anode voltage is 1000V.

• Proceedings of the Korea Society of Design Studies Conference
• /
• 2001.10a
• /
• pp.14.2-14
• /
• 2001

• Proceedings of the KIEE Conference
• /
• 1991.11a
• /
• pp.419-422
• /
• 1991

A mathematical model was developed to predict the temperature, the density, and the velocity distribution of an inductively coupled thermal plasma. It was for an atmospheric pressure argon thermal plasma generated by a 4 MHz radio frequency power. It has been shown that the hottest region can be moved toward centrial region by applying an external magnetic field. Based on the results of the simulation. an ICP(Inductively Coupled thermal Plasma) system was constructed and thermal plasma was generated.