• 제목/요약/키워드: astronomical observation

검색결과 721건 처리시간 0.029초

최근 천문학 연구 키워드와 천체 분야 교육과정 내용 요소 비교 분석 (A Comparative Analysis of Keywords in Astronomical Journals and Concepts in Secondary School Astronomy Curriculum)

  • 신현정;권우진;가석현
    • 한국과학교육학회지
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    • 제42권2호
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    • pp.289-309
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    • 2022
  • 힉스입자 발견, 블랙홀 이미지 촬영, 외계행성 탐사, 깊은 우주탐사, 중력파 관측 등 최근 천문학은 매우 빠르게 성장하고 있으며, 학생들도 상대적으로 흥미가 높은 분야이다. 본 연구의 목적은 최근 10년간 천문학 연구 저널에서 높은 빈도로 등장한 키워드들과 중고등학교 과학 교육과정에 포함된 천문학 내용 요소를 7개 영역별로 비교하여 천문학 교육과정 개선에 대한 시사점을 얻는 것이다. 우선 선정된 4개 저널-ApJ, ApJL, A&A, MNRAS-에 2011년부터 2020년까지 게재된 모든 논문의 키워드를 R 패키지로 수집하여 연구 동향을 살펴보았다. 교육과정 내용 요소는 7학년부터 12학년 학생이 배우는 과목 중 천문학 내용 요소가 포함된 6개 과목(과학, 통합과학, 지구과학I, 지구과학II, 물리II, 융합과학)의 2015 개정 교육과정 문서에 제시된 내용 체계표, 성취기준, 성취기준해설을 현직 교사들이 코딩한 결과를 종합하여 추출하였다. 연구 결과는 다음과 같다. 첫째, 천문학에서 꾸준하게 많이 등장하는 키워드는 'galaxies: formation, galaxies: active, star: formation, accretion, accretion discs, method: numerical'이다. 둘째, 천문학 교육과정은 모든 학생이 배우는 공통 과학 과목 안에서 'High Energy Astrophysical Phenomena' 영역을 제외한 모든 영역을 포함하도록 구성되었으나 키워드 수준에서 보면 과목별, 학년별 내용 요소 배치와 새롭게 도입할 만한 주제에 대한 검토가 필요한 것으로 나타났다. 본 연구는 과목의 근간을 이루는 과학연구 분야와 교육과정을 비교한 탐색적 연구로서, 연구 결과는 향후 천문학 교육과정 개정에 시사점을 줄 수 있는 기초 연구가 되길 기대한다.

劉河間의 運氣論과 그 運用에 관한 硏究 (A Study of Hagan's Ungi(河間運氣) theory and its application to modern society)

  • 이동호;박찬국
    • 대한한의학원전학회지
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    • 제13권2호
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    • pp.107-107
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    • 2000
  • 1. Ounyukki(五運六氣) theory was first developed from observation of astronomical phenomena. Natural phenomena were explained and incorporated into the concepts of Yukki(六氣), and Ohaeng(五行, the concept that all matter in the world are comprised of five fundamental elements), during Chon-guk(戰國) and Han(漢) periods. In that period. Kanji(干支, the method to present time with ten and twelve different kinds of symbol's combinations) was used to record Ounyukki(五運六氣). Theoretical study of Un-gi(運氣, the abbreviation of Ounyukki) was almost completed in Un-gichilpyon(運氣七篇) of Naekyong(內經). Un-gi(運氣) theory was further studied and considered to be very important socially, as well as medically, in Tang(唐), Song(宋), Kum(金), and Won(元) periods. Hagan(河間) published various studies based on Un-gi(運氣) theory in Kum won(金元) periods. 2. Hagan(河間) realized the limitation of a remedy method, of Sanghan(傷寒) theory. Therefore, he made an assumption that the prevalence of diseases in his period are closely related to Hwayol(火熱, a fire and a super-heat; two things out of Yukki(六氣)). His new theory was a result of the study on Kyongjon(經典, bibles of the oriental medicine) and the phenomena of nature. 3. Hagan(河間) used a combination of two basic theories of Pimuripsang(比物立象) and Hanhaesungjeron(亢害承制論) to make understood Hwayol(火熱) theory, Pimuripsang(比物立象) theory explains a method to appreciate the essence of things by comparing Sang(象, an expression of how something appears on the outside) and then making another Sang(象) from the comparison. Hanhaesungjeron(亢害承制論) is a theory to emphasize the importance of a balance of Yukki(六氣). It is that, if one of the elements is exceeded, other thing in the other five elements dominate the exceeded thing to control it for the balance between Yukki(六氣). In addition, he articulated P'yobon(標本. inside and outside of a thing) theory to differentiate the disease symptoms. These theories will help to distinguish real and fake symptoms of diseases, on which Hagan(河間) emphasized its importance. 4. Hagan(河間) published a new theory to explain Ounyukki(五運六氣) theory based on the observation of the nature and the experience from medical practice. And he added Chobyonggi(燥病機, course and rule causing disease in dry conditions) to Pyonggishipkujo(病機十九條, nineteen course and rule causing disease), it strengthened Pyonggi(病機, course and rule causing disease) theories. Moreover. he utilized Un-gi (運氣) theory in a real life situation by applying Un-giron(運氣論) to diagnosis like Maekchin(脈診, a method to diagnose by taking the pulse) and to prescription. 5. Modern society is an era in which it is hard to appreciate the principles of the changes due to the various unusual weather. Therefore, it is necessary to make a new paradigm using Un-gi(運氣) theory, like Hagan(河間) did in Kumwon(金元) period. 6. Unusual weather changes and the geriatric diseases such as cancer and diabetes, may have Sang(象) of Hwayol(火熱) theory at the other side. These diseases have been and will create more serious problems in modern society. As a method to solve these problems. it seems to be very important to understand and apply Hagan's(河間) Hawyol(火熱) theory to modern society.

유하간(劉河間)의 운기론(運氣論)과 그 운용(運用)에 관한 연구(硏究) (A study of Hagan's Ungi(河間運氣) theory and its application to modern society)

  • 이동호;박찬국
    • 대한한의학원전학회지
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    • 제13권2호
    • /
    • pp.108-145
    • /
    • 2000
  • 1. Ounyukki(五運六氣) theory was first developed from observation of astronomical phenomena. Natural phenomena were explained and incorporated into the concepts of Yukki(六氣), and Ohaeng(五行, the concept that all matter in the world are comprised of five fundamental elements), during Chon-guk(戰國) and Han(漢) periods. In that period. Kanji(干支, the method to present time with ten and twelve different kinds of symbol's combinations) was used to record Ounyukki(五運六氣). Theoretical study of Un-gi(運氣, the abbreviation of Ounyukki) was almost completed in Un-gichilpyon(運氣七篇) of Naekyong(內經). Un-gi(運氣) theory was further studied and considered to be very important socially, as well as medically, in Tang(唐), Song(宋), Kum(金), and Won(元) periods. Hagan(河間) published various studies based on Un-gi(運氣) theory in Kum won(金元) periods. 2. Hagan(河間) realized the limitation of a remedy method, of Sanghan(傷寒) theory. Therefore, he made an assumption that the prevalence of diseases in his period are closely related to Hwayol(火熱, a fire and a super-heat; two things out of Yukki(六氣)). His new theory was a result of the study on Kyongjon(經典, bibles of the oriental medicine) and the phenomena of nature. 3. Hagan(河間) used a combination of two basic theories of Pimuripsang(比物立象) and Hanhaesungjeron(亢害承制論) to make understood Hwayol(火熱) theory, Pimuripsang(比物立象) theory explains a method to appreciate the essence of things by comparing Sang(象, an expression of how something appears on the outside) and then making another Sang(象) from the comparison. Hanhaesungjeron(亢害承制論) is a theory to emphasize the importance of a balance of Yukki(六氣). It is that, if one of the elements is exceeded, other thing in the other five elements dominate the exceeded thing to control it for the balance between Yukki(六氣). In addition, he articulated P'yobon(標本. inside and outside of a thing) theory to differentiate the disease symptoms. These theories will help to distinguish real and fake symptoms of diseases, on which Hagan(河間) emphasized its importance. 4. Hagan(河間) published a new theory to explain Ounyukki(五運六氣) theory based on the observation of the nature and the experience from medical practice. And he added Chobyonggi(燥病機, course and rule causing disease in dry conditions) to Pyonggishipkujo(病機十九條, nineteen course and rule causing disease), it strengthened Pyonggi(病機, course and rule causing disease) theories. Moreover. he utilized Un-gi (運氣) theory in a real life situation by applying Un-giron(運氣論) to diagnosis like Maekchin(脈診, a method to diagnose by taking the pulse) and to prescription. 5. Modern society is an era in which it is hard to appreciate the principles of the changes due to the various unusual weather. Therefore, it is necessary to make a new paradigm using Un-gi(運氣) theory, like Hagan(河間) did in Kumwon(金元) period. 6. Unusual weather changes and the geriatric diseases such as cancer and diabetes, may have Sang(象) of Hwayol(火熱) theory at the other side. These diseases have been and will create more serious problems in modern society. As a method to solve these problems. it seems to be very important to understand and apply Hagan's(河間) Hawyol(火熱) theory to modern society.

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광해에 따른 밤하늘의 밝기 변화를 중심으로 본 천문 관측 환경 (Astronomical Observation Environment Study focusing on Night Sky Brightness Variation under Light Pollution)

  • 이진희;최승언;정재훈;우홍균
    • 한국지구과학회지
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    • 제30권3호
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    • pp.344-353
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    • 2009
  • 광해의 정도를 알아보기 위해 서울대 사범대학 주변 밤하늘의 밝기를 측정하였다. 표준성을 이용하여 고도에 따른 소광 계수 및 영점 상수를 구한 결과, 2009년 1월 28일에는 소광계수가 $k_B$=0.359, 영점상수는 $C_B$=4.397이 었고, 2009년 3월 27일에는 소광계수가 $k_B$=0.896, $k_V$=0.725, 영점상수는 $C_B$=6.235, $C_V$=6.027이었다. 밤하늘의 밝기는 동, 서, 남, 북 네 방위에 대해 고도 $20^{\circ}$, $40^{\circ}$, $60^{\circ}$, $75^{\circ}$, $90^{\circ}$에서 측정하였다. IRAF를 사용하여 전처리하고 측광한 결과, 1월 28일의 시상은 평균 5.1"였고 3월 27일은 5.7"이었다. 밤하늘의 등급은 방위 및 고도에 따라 $16{\leq}m_V$, $m_B{\leq}18$이었다. 도심 방향의 밤하늘 밝기는 어두운 지역에 비해 2-4정도 밝게 나타났다. 이러한 관측 조건에서 구경 40cm인 망원경을 통해 육안으로 관측할 수 있는 한계 등급은 밤하늘의 밝기 정도에 따라 대략 11-13등급이다. 1월과 3월의 밤하늘 밝기를 비교해 본 결과, B필터에서 1월이 3월에 비해 1등급 정도 어두운 것으로 나타났다.

수치표고모델, 3차원 카메라이미지자료 및 복사모델을 이용한 Sky Line과 Skyview Factor에 따른 강릉원주대학교 복사관측소 관측환경 분석 (Analysis of Observation Environment with Sky Line and Skyview Factor using Digital Elevation Model (DEM), 3-Dimensional Camera Image and Radiative Transfer Model at Radiation Site, Gangneung-Wonju National University)

  • 지준범;조일성;김부요;이규태;장정필
    • 대기
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    • 제29권1호
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    • pp.61-74
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    • 2019
  • To investigate the observational environment, sky line and skyview factor (SVF) are calculated using a digital elevation model (DEM; 10 m spatial resolution) and 3 dimensional (3D) sky image at radiation site, Gangneung-Wonju National University (GWNU). Solar radiation is calculated using GWNU solar radiation model with and without the sky line and the SVF retrieved from the 3D sky image and DEM. When compared with the maximum sky line elevation from Skyview, the result from 3D camera is higher by $3^{\circ}$ and that from DEM is lower by $7^{\circ}$. The SVF calculated from 3D camera, DEM and Skyview is 0.991, 0.998, and 0.993, respectively. When the solar path is analyzed using astronomical solar map with time, the sky line by 3D camera shield the direct solar radiation up to $14^{\circ}$ with solar altitude at winter solstice. The solar radiation is calculated with minutely, and monthly and annual accumulated using the GWNU model. During the summer and winter solstice, the GWNU radiation site is shielded from direct solar radiation by the west mountain 40 and 60 minutes before sunset, respectively. The monthly difference between plane and real surface is up to $29.18M\;m^{-2}$ with 3D camera in November, while that with DEM is $4.87M\;m^{-2}$ in January. The difference in the annual accumulated solar radiation is $208.50M\;m^{-2}$ (2.65%) and $47.96M\;m^{-2}$ (0.63%) with direct solar radiation and $30.93M\;m^{-2}$ (0.58%) and $3.84M\;m^{-2}$ (0.07%) with global solar radiation, respectively.

천문 교구를 활용한 HTE-STEAM 별자리 교육 프로그램 개발 연구 : 시공간 개념을 통한 미래 사회 핵심역량 함양을 중심으로 (Development of HTE-STEAM Constellation Education Program Using Astronomical Teaching Aid: Focused on Cultivating Core Competencies for Future Society through the Concept of Space and Time)

  • 조아라;김용기
    • 대한지구과학교육학회지
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    • 제17권1호
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    • pp.34-48
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    • 2024
  • 세계적으로 역량중심 교육이 주목됨에 따라, 교육부는 2015 개정 교육과정에서 창의융합형 인재가 갖춰야 할 미래 사회 핵심역량 6가지를 제시하였다. 본 연구에서는 2015 개정 교육과정에 제시된 미래 사회 핵심역량을 함양하고, 천문 영역 실험·실습의 한계를 보완하기 위해 HTE-STEAM 별자리 교육 프로그램을 개발하였고 그 효율성을 파일럿 테스트를 통해 확인하였다. 개발한 프로그램은 학교 밖 교육 현장인, 충청북도 청주시 소재의 G 도서관에서 초등 3~6학년 학생들을 대상으로 적용하였다. 연구의 결과는 다음과 같다. 첫째, HTE-STEAM 별자리 교육 프로그램은 STEAM 태도 검사의 '자아 개념'을 제외한 모든 구인에서 통계적으로 유의미한 효과를 보였으며, 특히 '이공계 진로선택', '배려', '소통'에서 높은 효과를 보였다. 따라서 미래 사회 핵심역량 중 '창의적 사고 역량'과 '의사소통 역량', '공동체 역량'의 함양에 긍정적인 결과를 도출하였다. 둘째, HTE-STEAM 별자리 교육 프로그램은 시공간이라는 어려운 개념을 다루었으나, 수업 내용의 난이도가 쉽다고 응답한 학생들이 많고, 배운 공간개념을 응용하여 교구를 활용한 것으로 보아, 학생들의 하늘과 우주의 공간 구조에 대한 이해에 효과적이었다. 덧붙여, 본 프로그램은 2022 개정 교육과정에서 추가된 하늘의 공간적 구조에 대한 성취기준을 충족하는 교육 프로그램으로 활용될 수 있을 것으로 보인다. 따라서 HTE-STEAM을 기반으로 한 별자리 교육 프로그램은 미래 사회 핵심 역량의 함양에 긍정적인 효과를 보였으며, 학교 환경에서 천문 영역의 야간 관측 실습을 보완하는 역할을 할 수 있을 것으로 보인다.

우주전파 관측을 위한 광대역 음향광학 전파분광기 설계 (Design of a Wide-band Acousto-Optical Spectrometer for Radio Astronomical Observations)

  • 임인성;민경일;오승엽
    • 한국전자파학회논문지
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    • 제12권6호
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    • pp.1009-1017
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    • 2001
  • 우주전파의 신호를 관측하기 위한 1 GHz대역의 음향광학 전파분광기를 설계.제작하였다. 이 전파분광기는 다중채널 방식의 신호의 세기가 미약한 우주 전파신호를 분석하기 위한 초고감도의 전파 분광기로, 관측되는 스펙트럼의 모양을 상세히 측정할 수 있는 전파분광기이다. 주파수 분해능과 광대역 주파수 성분을 포함하는 이 음향광학 전파분광기의 광원(optical source)으로는 He-Ne 레이저를 사용하였고, 1 GHz에서 2 GHz까지의 대역폭을 갖는 광대역 GaP 광펼향 소자를 사용하였으며, 광신호 검출을 위해 2,048 채널의 CCD를 사용하였다. 전파망원경을 통해 우주전파신호인 CRL 2688, IRC 10216 그리고 NGC 5005 은하 중심의 12CO(J= 1 ~0) 분자선(molecular line)을 관측한 결과, 광대역의 특성을 가지며 주파수 분해능이 양호함을 확인하였다.

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Recent Progress of MIRIS Development

  • Han, Won-Yong;Lee, Dae-Hee;Park, Young-Sik;Nam, Uk-Won;Jeong, Woong-Seob;Ree, Chang-Hee;Moon, Bong-Kon;Park, Sung-Joon;Cha, Sang-Mok;Lee, Duk-Hang;Park, Jang-Hyun;;Seon, Kwang-Il;Yang, Sun-Choel;Park, Jong-Oh;Rhee, Seung-Wu;Lee, Hyung-Mok;Matsumoto, Toshio
    • 한국우주과학회:학술대회논문집(한국우주과학회보)
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    • 한국우주과학회 2011년도 한국우주과학회보 제20권1호
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    • pp.23.4-23.4
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    • 2011
  • MIRIS is the main payload of the Science and Technology Satellite-3 (STSAT-3). which is being developed by KASI for infrared survey observation of the Galactic plane at Paschen alpha wavelength. Wideband filters in I and H band will also be used to observe cosmic infrared background. The MIRIS will perform astronomical observations in the near-infrared wavelengths of 0.9~2 ${\mu}m$ using a 256 ${\times}$ 256 Teledyne PICNIC FPA sensor providing a 3.67 ${\times}$ 3.67 degree field of view with a pixel scale of 51.6 arcsec. The flight model of the MIRIS has been recently developed, The system performance tests have been made in the laboratory, including opto-mechanics test, vibration test, thermal vacuum test and passive cooling test down to 200K, using a thermally controlled vacuum chamber. Several focus tests showed good agreements compared to initial design parameters. Recent efforts are being concentrated to improve the system performances, particularly to reduce readout noise level in electronics. After assembly and integration into the satellite bus, the MIRIS will be launched in 2012.

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Performance Analysis for Mirrors of 30 cm Cryogenic Space Infrared Telescope

  • Park, Kwi-Jong;Moon, Bong-Kon;Lee, Dae-Hee;Jeong, Woong-Seob;Nam, Uk-Won;Park, Young-Sik;Pyo, Jeong-Hyun;Han, Won-Yong
    • Journal of Astronomy and Space Sciences
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    • 제29권3호
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    • pp.321-328
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    • 2012
  • We have designed a 30 cm cryogenic space infrared telescope for astronomical observation. The telescope is designed to observe in the wavelength range of 0.5~2.1 ${\mu}m$, when it is cooled down to 77 K. The result of the preliminary design of the support structure and support method of the mirror of a 30 cm cryogenic space infrared telescope is shown in this paper. As a Cassegrain prescription, the optical system of a 30 cm cryogenic space infrared telescope has a focal ratio of f/3.1 with a 300 mm primary mirror (M-1) and 113 mm secondary mirror (M-2). The material of the whole structure including mirrors is aluminum alloy (Al6061-T6). Flexures that can withstand random vibration were designed, and it was validated through opto-mechanical analysis that both primary and secondary mirrors, which are assembled in the support structure, meet the requirement of root mean square wavefront error < ${\lambda}/8$ for all gravity direction. Additionally, when the M-1 and flexures are assembled by bolts, the effect of thermal stress occurring from a stainless steel bolt when cooled and bolt torque on the M-1 was analyzed.

An Application of Hilbert-Huang Transform on the Non-Stationary Astronomical Time Series: The Superorbital Modulation of SMC X-1

  • Hu, Chin-Ping;Chou, Yi;Wu, Ming-Chya;Yang, Ting-Chang;Su, Yi-Hao
    • Journal of Astronomy and Space Sciences
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    • 제30권2호
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    • pp.79-82
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    • 2013
  • We present the Hilbert-Huang transform (HHT) analysis on the quasi-periodic modulation of SMC X-1. SMC X-1, consisting of a neutron star and a massive companion, exhibits superorbital modulation with a period varying between ~40 d and ~65 d. We applied the HHT on the light curve observed by the All-Sky Monitor onboard Rossi X-ray Timing Explorer (RXTE) to obtain the instantaneous frequency of the superorbital modulation of SMC X-1. The resultant Hilbert spectrum is consistent with the dynamic power spectrum while it shows more detailed information in both the time and frequency domains. According to the instantaneous frequency, we found a correlation between the superorbital period and the modulation amplitude. Combining the spectral observation made by the Proportional Counter Array onboard RXTE and the superorbital phase derived in the HHT, we performed a superorbital phase-resolved spectral analysis of SMC X-1. An analysis of the spectral parameters versus the orbital phase for different superorbital states revealed that the diversity of $n_H$ has an orbital dependence. Furthermore, we obtained the variation in the eclipse profiles by folding the All Sky Monitor light curve with orbital period for different superorbital states. A dip feature, similar to the pre-eclipse dip of Her X-1, can be observed only in the superorbital ascending and descending states, while the width is anti-correlated with the X-ray flux.