• Title/Summary/Keyword: energy space

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Space Weather and Relativistic Electron Enhancement

  • Lee, J.J.;Parks, G.K.;McCarthy, M.P.;Min, K.W.;Lee, E.S.;Kim, H.J.;Park, J.H.;Hwang, J.A.
    • Bulletin of the Korean Space Science Society
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    • 2006.10a
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    • pp.52-52
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    • 2006
  • Many spacecraft failures and anomalies have been attributed to energetic electrons in the Earth's magnetosphere. While the dynamics of these electrons have been studied extensively for several decades, the fundamental question of how they are accelerated is not fully resolved. Proposed theories have not been successful in explaining fast high energy increase such as REE (Relativistic electron enhancement). In this presentation, we show observations of energetic electron precipitation measured by the Korean satellite, STSAT-1 which simultaneously detect (100ev - 20 keV) and (170 - 360 keV) energy electrons at the 680 km orbit, when the RES event observed at the geosynchronous orbit on October 13, 2004. STSAT-1 observed intense electron precipitation in both energy ranges occurred in the midnight sector clearly demonstrating that electrons having wide energy band are injected from the plasma sheet. To make the balance between loss and injection, the injected electron flux should be also large. In this situation, the injected electrons can be trapped into the magnetosphere and produce REE, though they have low e-folding energies. We propose this plasma sheet injection might be the primary source of relativistic electron (1 MeV) flux increases.

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EVALUATION OF SURFACE HEAT FLUXES FOR DIFFERENT LAND COVER IN HEAT ISLAND EFFECT

  • Chang, Tzu-Yin;Liao, Lu-Wei;Liou, Yuei-An
    • Proceedings of the KSRS Conference
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    • 2008.10a
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    • pp.68-71
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    • 2008
  • Our goal is to obtain a better scientific understanding how to define the nature and role of remotely sensed land surface parameters and energy fluxes in the heat island phenomena, and local and regional weather and climate. By using the MODIS visible and thermal imagery data and analyzing the surface energy flux images associated with the change of the landcover and landuse in study area, we will estimate and present how significant is the magnitude of the heat island heat effect and its relation with the surface parameters and the energy fluxes in Taiwan. To achieve our objective, we used the energy budget components such as net radiation, soil heat flux, sensible heat flux, and latent heat flux in the study area of interest derived form remotely sensed data to understand the island heat effect. The result shows that the water is the most important component to decrease the temperature, and the more the consumed net radiation to latent heat, the lower urban surface temperature.

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A Study on the Air System for Space Heating (공기식 집열시스템에 의한 실내 난방 연구)

  • Chun, Won-Gee;Lim, Sang-Hoon;Jeon, Myung-Seok;Yoon, Jong-Ho
    • Solar Energy
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    • v.12 no.1
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    • pp.34-39
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    • 1992
  • The present study has carried out thermal performance evaluation of air systems for space heating in Daejeon by the f-chart method. The various effects with the change in air flow rate, number of glazings, storage capacity of pebble bed, and coating materials of absorber plate are analyzed with regard to the effectiveness of air systems for space heating. A comparison is also made with liquid systems under the same operating conditions.

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A comparison study of CORSIKA and COSMOS simulations for extensive air showers

  • Kim, Ji-Hee;Roh, Soon-Young;Ryu, Dong-Su;Kang, Hye-Sung
    • The Bulletin of The Korean Astronomical Society
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    • v.37 no.1
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    • pp.69.1-69.1
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    • 2012
  • Monte Carlo codes for extensive air shower (EAS) simulate the development of EASs initiated in the Earth's atmosphere by ultra-high energy cosmic rays (UHECRs) with energy exceeding - $10^{18}$ eV. Here, we compare EAS simulations with two different codes, CORSIKA and COSMOS, presenting quantities including the longitudinal distribution of particles, depth of shower maximum, kinetic energy distribution of particle at the ground, and calorimetric energy. In addition, the lateral distribution of local energy density far from the EAS core has been known as an important quantity to estimate the energy of UHECRs. We also present the lateral distribution function obtained from GEANT4 simulations for detector response.

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High-energy Photons and Particles in Space Environment

  • Ohno, Shin-ichi
    • Journal of Photoscience
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    • v.9 no.2
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    • pp.170-173
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    • 2002
  • Space is full of energetic events emitting high-energy radiations which may be fatal to all living things unless protected. The present paper briefly describes high-energy photons and particles incident on Earth surface and their common properties toward living things. Role of radiation played in evolution of life and earth environment will be presented.

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A Study on Stability of Single-layer Space Frame Structure for Energy Core of Incheon Airport Second Terminal (인천공항 제2터미널 에너지코어 단층 스페이스 프레임 구조물의 안정에 관한 연구)

  • Jung, Hwan-Mok
    • Journal of Korean Association for Spatial Structures
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    • v.15 no.4
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    • pp.49-56
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    • 2015
  • The roof grid of single-layer space frame structure, for Energy Core of Incheon Airport Second Terminal, is very simple and aesthetic, but it is apt to buckle under external force because of mild curvature and complex shape. The object of this study is to estimate the stability of single-layer space frame structures for Energy Core of Incheon Airport Second Terminal with the analytical conditions of structural design. The results show that the buckling load of model(pin-pin, uniform load, rigid joint), that is, the most similar model to the analytical conditions of structural design. was $10.7kN/m^2$.

Development of High Energy Particle Detector for the Study of Space Radiation Storm

  • Jo, Gyeong-Bok;Sohn, Jongdae;Choi, Cheong Rim;Yi, Yu;Min, Kyoung-Wook;Kang, Suk-Bin;Na, Go Woon;Shin, Goo-Hwan
    • Journal of Astronomy and Space Sciences
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    • v.31 no.3
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    • pp.277-283
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    • 2014
  • Next Generation Small Satellite-1 (NEXTSat-1) is scheduled to launch in 2017 and Instruments for the Study of Space Storm (ISSS) is planned to be onboard the NEXTSat-1. High Energy Particle Detector (HEPD) is one of the equipment comprising ISSS and the main objective of HEPD is to measure the high energy particles streaming into the Earth radiation belt during the event of a space storm, especially, electrons and protons, to obtain the flux information of those particles. For the design of HEPD, the Geometrical Factor was calculated to be 0.05 to be consistent with the targets of measurement and the structure of telescope with field of view of $33.4^{\circ}$ was designed using this factor. In order to decide the thickness of the detector sensor and the classification of the detection channels, a simulation was performed using GEANT4. Based on the simulation results, two silicon detectors with 1 mm thickness were selected and the aluminum foil of 0.05 mm is placed right in front of the silicon detectors to shield low energy particles. The detection channels are divided into an electron channel and two proton channels based on the measured LET of the particle. If the measured LET is less than 0.8 MeV, the particle belongs to the electron channel, otherwise it belongs to proton channels. HEPD is installed in the direction of $0^{\circ}$, $45^{\circ}$, $90^{\circ}$ against the along-track of a satellite to enable the efficient measurement of high energy particles. HEPD detects electrons with the energy of 0.1 MeV to several MeV and protons with the energy of more than a few MeV. Thus, the study on the dynamic mechanism of these particles in the Earth radiation belt will be performed.

SIMULATION OF THE TISSUE EQUIVALENT PROPORTIONAL COUNTER IN THE INTERNATIONAL SPACE STATION WITH GEANT4 (Geant4를 활용한 국제우주정거장 내의 조직등가비례계수기 모의 실험)

  • Pyo, Jeong-Hyun;Lee, Jae-Jin;Nam, Uk-Won;Kim, Sung-Hwan;Kim, Hyun-Ok;Lim, Chang-Hwy;Park, Kwi-Jong;Lee, Dae-Hee;Park, Young-Sik;Moon, Myung-Kook
    • Publications of The Korean Astronomical Society
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    • v.27 no.3
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    • pp.81-86
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    • 2012
  • The International Space Station (ISS) orbits the Earth within the inner radiation belt, where high-energy protons are produced by collisions of cosmic rays to the upper atmosphere. About 6 astronauts stay in the ISS for a long period, and it should be important to monitor and assess the radiation environment in the ISS. The tissue equivalent proportional counter (TEPC) is an instrument to measure the impact of radiation on the human tissue. KASI is developing a TEPC as a candidate payload of the ISS. Before the detailed design of the TEPC, we performed simulations to test whether our conceptual design of the TEPC will work propertly in the ISS and to predict its performance. The simulations estimated that the TEPC will measure the dose equivalent of about 1:1 mSv during a day in the ISS, which is consistent with previous measurements.

The importance of nuclear energy for the expansion of world's energy demand

  • Guk, Erdogan;Kalkan, Naci
    • Advances in Energy Research
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    • v.3 no.2
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    • pp.71-80
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    • 2015
  • This paper describes nuclear energy technologies for the solution of long term energy problem with better reliability. A short overview about nuclear energy applications are explained with a basic analysis of energy. Furthermore, industrial application, space application of nuclear systems and ship propulsion in nuclear energy application are demonstrated in more detail. This report also includes some examples of the experienced nuclear power plant to identify energy production. The general purpose of the article is to understand how efficiently nuclear systems generates energy, and solve the world's increasing energy demand in our century.