• Title/Summary/Keyword: energy space

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A Study on Rockfall Energy and Rockfall Protection Fence Applications on the Slope (사면에서 발생하는 낙석에너지와 낙석방지울타리 적용성에 관한 연구)

  • 김남호;신윤섭;박윤재;조종석
    • Proceedings of the Korean Geotechical Society Conference
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    • 2002.03a
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    • pp.523-530
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    • 2002
  • Recently, while rockfall occurs very frequently, a lot of researches on the rockfall protection fence Is in process. But the rockfall protection fence has been installed unrelated to slope characteristics, rockfall shape and rockfall height. Therefore, in this study we suggested the effective protection fence model considering about rockfall energy and energy absorbing capacity and we verified the model by field test. According to these results, it is more reasonable to evaluate rockfall energy based on the results of simulation program, which can be consider effects of energy decrease, than use the simplified method proposed by Japanese road association. And rockfall energy is affected by the size of supports and wire rope and the space of supports. As the results of comparing rockfall energy with energy absorbing capacity, type$\circled1$(the space of supports is changed to 3.0m)can be available for generally expected rockfall except the rock slope over 30m heights. But rockfall protection fence installed at the field, it should be partially reinforced after consideration of slope particularities and construction conditions.

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Construction of Korean Space Weather Prediction Center: Space radiation effect

  • Lee, Jae-Jin;Cho, Kyung-Suk;Hwang, Jung-A;Kwak, Young-Sil;Kim, Khan-Hyuk;Bong, Su-Chan;Kim, Yeon-Han;Park, Young-Deuk;Choi, Seong-Hwan
    • Bulletin of the Korean Space Science Society
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    • 2008.10a
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    • pp.33.3-34
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    • 2008
  • As an activity of building Korean Space Weather Prediction Center (KSWPC), we has studied of radiation effect on the spacecraft components. High energy charged particles trapped by geomagnetic field in the region named Van Allen Belt can move to low altitude along magnetic field and threaten even low altitude spacecraft. Space Radiation can cause equipment failures and on occasions can even destroy operations of satellites in orbit. Sun sensors aboard Science and Technology Satellite (STSAT-1) was designed to detect sun light with silicon solar cells which performance was degraded during satellite operation. In this study, we try to identify which particle contribute to the solar cell degradation with ground based radiation facilities. We measured the short circuit current after bombarding electrons and protons on the solar cells same as STSAT-1 sun sensors. Also we estimated particle flux on the STSAT-1 orbit with analyzing NOAA POES particle data. Our result clearly shows STSAT-1 solar cell degradation was caused by energetic protons which energy is about 700 keV to 1.5 MeV. Our result can be applied to estimate solar cell conditions of other satellites.

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Nonthermal Radiation from Supernova Remnant Shocks

  • Kang, Hyesung
    • Journal of Astronomy and Space Sciences
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    • v.30 no.3
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    • pp.133-140
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    • 2013
  • Most of high energy cosmic rays (CRs) are thought to be produced by diffusive shock acceleration (DSA) at supernova remnants (SNRs) within the Galaxy. Fortunately, nonthermal emissions from CR protons and electrons can provide direct observational evidence for such a model and place strong constraints on the complex nonlinear plasma processes in DSA theory. In this study we calculate the energy spectra of CR protons and electrons in Type Ia SNRs, using time-dependent DSA simulations that incorporate phenomenological models for some wave-particle interactions. We demonstrate that the time-dependent evolution of the self-amplified magnetic fields, Alfv$\acute{e}$nic drift, and escape of the highest energy particles affect the energy spectra of accelerated protons and electrons, and so resulting nonthermal radiation spectrum. Especially, the spectral cutoffs in X-ray and ${\gamma}$-ray emission spectra are regulated by the evolution of the highest energy particles, which are injected at the early phase of SNRs. Thus detailed understandings of nonlinear wave-particle interactions and time-dependent DSA simulations of SNRs are crucial in testing the SNR hypothesis for the origin of Galactic cosmic rays.

Optimal design of a piezoelectric passive damper for vibrating plates

  • Yun, Chul-Yong;Kim, Seung-Jo
    • International Journal of Aeronautical and Space Sciences
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    • v.7 no.2
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    • pp.42-49
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    • 2006
  • In this paper, an efficient piezoelectric passive damper is newly devised to suppress the multi-mode vibration of plates. To construct the passive damper, the piezoelectric materials are utilized as energy transformer, which can transform the mechanical energy to electrical energy. To dissipate the electrical energy transformed from mechanical energy, multiple resonant shunted piezoelectric circuits are applied. The dynamic governing equations of a coupled electro-mechanical piezoelectric with multiple piezoelectric patches and multiple resonant shunted circuits is derived and solved for the one edge clamped plate. The equations of motion of the piezoelectrics and shunted circuits as well as the plate are discretized by finite element method to estimate more exactly the effectiveness of the piezoelectric passive damper. The method to find the optimal location of a piezoelectric is presented to maximize effectiveness for desired modes. The electro-mechanical coupling term becomes important parameter to select the optimal location.

In-Situ Diagnosis of Vapor-Compressed Chiller Performance for Energy Saving

  • Shin Younggy;Kim Youngil;Moon Guee-Won;Choi Seok-Weon
    • Journal of Mechanical Science and Technology
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    • v.19 no.8
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    • pp.1670-1681
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    • 2005
  • In-situ diagnosis of chiller performance is an essential step for energy saving business. The main purpose of the in-situ diagnosis is to predict the performance of a target chiller. Many models based on thermodynamics have been proposed for the purpose. However, they have to be modified from chiller to chiller and require profound knowledge of thermodynamics and heat transfer. This study focuses on developing an easy-to-use diagnostic technique that is based on adaptive neuro-fuzzy inference system (ANFIS). The effect of sample data distribution on training the ANFIS is investigated. It is found that the data sampling over 10 days during summer results in a reliable ANFIS whose performance prediction error is within measurement errors. The reliable ANFIS makes it possible to prepare an energy audit and suggest an energy saving plan based on the diagnosed chilled water supply system.

THE ELECTRON FRACTION AND THE FERMI ENERGY OF RELATIVISTIC ELECTRONS IN A NEUTRON STAR

  • GAO, ZHI FU;LI, X.D.;WANG, N.;PENG, Q.H.
    • Publications of The Korean Astronomical Society
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    • v.30 no.2
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    • pp.569-572
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    • 2015
  • We first deduce a uniform formula forthe Fermi energy of degenerate and relativistic electrons in the weak-magnetic field approximation. Then we obtain an expression of the special solution for the electron Fermi energy through this formula, and express the electron Fermi energy as a function of electron fraction and matter density. Our method is universally suitable for relativistic electron- matter regions in neutron stars in the weak-magnetic field approximation.

Effect of two-temperature on the energy ratio at the boundary surface of inviscid fluid and piezothermoelastic medium

  • Kumar, Rajneesh;Sharma, Poonam
    • Earthquakes and Structures
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    • v.18 no.6
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    • pp.743-752
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    • 2020
  • The phenomenon of reflection and transmission of plane waves at an interface between fluid half space and orthotropic piezothermoelastic solid half-space with two-temperature has been investigated. Energy ratios of various reflected and transmitted waves are computed with the use of amplitude ratios. The law of conservation of energy across the interface has been justified. It is found that the energy ratios are the functions of angle of incidence, frequency of independent wave and depend on the different piezothermoelastic material. A piezothermoelastic material has been considered which is in welded contact with water. Variations of energy ratios corresponding to the reflected waves and transmitted waves are computed and shown graphically for the two different models. A particular reduced case of interest is also discussed.

Characteristics and Research Trend of Agrivoltaics (영농형 태양광 발전시스템의 특성 및 연구동향)

  • Seok Jin Jang;Jinjoo Park;Junsin Yi
    • Current Photovoltaic Research
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    • v.12 no.3
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    • pp.74-79
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    • 2024
  • Photovoltaics (PV) is gaining attention as an alternative energy source to fossil fuels. Although the demand for PV is increasing, it requires more than three times the space compared to conventional power generation, leading to limtation of available land for PV installations. Agrivoltaics is combined with agriculture and solar power generation at the same space, making it highly efficient in terms of land use. This review explores various forms of agrivoltaics systems currently being researched and examines the relationship between energy production and agricultural productivity in these systems. With agrivoltaics, about 70-80% of the energy production of conventional solar power can be achieved, while agricultural yields can reach up to 90% of those produced through conventional farming methods.

Analysis on Characteristics of Thermal Flow for Heating Indoor Space by Air-heating Collector using Solar Heat (태양열 공기가열 집열기에 의한 난방 실내공간의 열유동 특성 해석)

  • Yang, Young-Joon
    • Journal of the Korean Society of Industry Convergence
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    • v.25 no.2_2
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    • pp.271-278
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    • 2022
  • The solar energy has been widely used to reduce the fossil fuel and prevent the environmental pollution. The renewable energy including solar heat tends to spread due to carbon neutrality for main country of the world. Targets of solar collector are usually acquisitions of hot water or hot air. Especially, air-heating collector using solar heat is known as the technology for obtaining hot air. This study aims to investigate of characteristics of thermal flow when the hot air by air-heating collector using solar heat flows inside of indoor space. The thermal flow of heating indoor space was simulated using ANSYS-CFX program and thus the behaviors of hot air in indoor space were evaluated with standard k-𝜀 turbulence model. As the results, as the inlet velocity was increased, the behaviors of hot air became simple, and temperature range of 25~75℃ had almost no effect on behavior of flow. As the inlet temperature was increased, the temperature curve of indoor space from bottom to top was changed from linear to quadratic. Furthermore, it was confirmed that inlet velocity as well as inlet temperature also should be considered to heat indoor space equally by air-heating collector using solar heat.

Space Radiation Effect on Si Solar Cells (우주 방사능에 의한 실리콘 태양 전지의 특성 변화)

  • Lee, Jae-Jin;Kwak, Young-Sil;Hwang, Jung-A;Bong, Su-Chang;Cho, Kyung-Seok;Jeong, Seong-In;Kim, Kyung-Hee;Choi, Han-Woo;Han, Young-Hwan;Choi, Yong-Woon;Seong, Baek-Il
    • Journal of Astronomy and Space Sciences
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    • v.25 no.4
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    • pp.435-444
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    • 2008
  • High energy charged particles are trapped by geomagnetic field in the region named Van Allen Belt. These particles can move to low altitude along magnetic field and threaten even low altitude spacecraft. Space Radiation can cause equipment failures and on occasions can even destroy operations of satellites in orbit. Sun sensors aboard Science and Technology Satellite (STSAT-l) was designed to detect sun light with silicon solar cells which performance was degraded during satellite operation. In this study, we try to identify which particle contribute to the solar cell degradation with ground based radiation facilities. We measured the short circuit current after bombarding electrons and protons on the solar cells same as STSAT-1 sun sensors. Also we estimated particle flux on the STSAT-l orbit with analyzing NOAA POES particle data. Our result clearly shows STSAT-l solar cell degradation was caused by energetic protons which energy is about 700keV to 1.5MeV. Our result can be applied to estimate solar cell conditions of other satellites.