이 연구는 ‘태양 복사’가 ‘가시광선 복사’로, ‘지구 복사’가 ‘적외선 복사’로 상호 대체될 수 있는 개념인가에 대한 문제 인식에서 출발하였다. 이를 위해 각 개념을 어떻게 인식하고 있는지를 드러낼 수 있는 질문지를 통하여 지 구과학 I을 이수한 고등학생들의 인식을 조사하고, 이들의 인식에 영향을 미칠 수 있는 교과서의 서술 및 삽화를 분석 하였다. 이 연구의 주요 결과는 다음과 같다. 첫째, 조사에 참여한 학생들은 모두 태양 복사를 가시광선 영역에서만 방출되는 복사로 인식하고 있으며, 지구 열수지에서 대류·전도·숨은열을 복사에 의한 에너지 전달로 인식하고 있는 학생 들도 약 35%로 나타났다. 둘째, 2015 개정 교육과정의 지구과학 I 6종 교과서를 분석한 결과, 2종에서는 ‘단파 복사’와 ‘장파 복사’라는 용어를 도입하지만 이들에 대한 설명이 없었으며, 다른 2종에서는 태양 복사를 각각 ‘주로 가시광선 형 태의 복사’ 또는 ‘파장이 짧은 가시광선 복사’로 서술하였다. 그 밖의 2종 교과서에 있는 태양 복사와 지구 복사에 관 하여, 파장 영역에 대한 설명이 없거나 ‘단파장/장파장’이라는 모호한 용어가 사용되었다. 아울러 2종의 교과서에서 열 수지 삽화에 일부 오류가 발견되었다. 따라서 교과서들이 단파 복사와 장파 복사에 관한 정확한 용어 정의 없이 태양 복사와 지구 복사를 설명함에 따라 학습자들은 태양 복사와 지구 복사를 각각 가시광선 복사와 적외선 복사라는 개념 으로 인식할 개연성이 있다. 이를 종합해 보면, 교과서에 기술된 불분명한 진술이나 오류가 학생들의 오개념을 유발하 거나 재생산할 수 있음을 함의한다. 이 연구에서 논의된 바가 지구의 열수지와 복사 평형에 대한 교수·학습 과정의 유 용한 참고 자료로 활용되고, 추후 교과서 집필에서도 합리적인 서술 방안을 제안하는 데 기여할 수 있으리라 기대한다.

First light galaxies have predictable linear clustering, and are expected to produce fluctuations with a characteristic spatial power spectrum, which peaks at an angular scale of ~ 10 arcminutes and in the 1―2 μm spectral regions. The Cosmic Infrared Background ExpeRiment 2 (CIBER2) is a dedicated sounding rocket mission for measuring the fluctuations in the extragalactic infrared background light, following up the previous successful measurements of CIBER1. With a 28.5 cm telescope accompanied with three arms of camera barrels and a dual broadband filter on each H2RG (λc = 2.5 μm) array, CIBER2 can measure 6 bands of wide field (1.1 × 2.2 degrees) up to 3 AB magnitudes deeper than CIBER1. This project is leaded by California Institute of Technology/Jet Propulsion Laboratory, collaborating internationally with Institute of Space and Astronautical Science in Japan, Korea Astronomy and Space Science Institute, Korea Basic Science Institute, and Seoul National University. The Korean team is in charge of 1) one H2RG scientific array, 2) ground station hardware and software, 3) telescope lenses, and 4) flight and test bed electronics fabrication. In this paper, we describe the detailed activities of the Korean participation as well as the current status of the CIBER2 project.

We present the sensitivity calculation results for observing the Cosmic Infrared Background (CIRB) by the Multi-purpose IR Imaging System (MIRIS), which will be launched in 2010 as a main payload of the Science and Technology Satellite 3 (STSAT-3). MIRIS will observe in I ( 0.9∼1.2um) and H (1.2∼2.0um) band with a 4×4 degree field of view to obtain the large scale structure ( ∼3 degree) of the CIRB. With the given specifications of the MIRIS, our sensitivity calculation results show that the MIRIS has a detection limit of ∼9nWm−2sr−1 (I band) and ∼6nWm−2sr−1 (H band), which is appropriate to observe the large scale structure of CIRB.

The international cooperation project CIBER (Cosmic Infrared Background ExpeRiment) is a rocket-borne instrument, of which the scientific goal is to measure the cosmic near-infrared extra-galactic background to search for signatures of primordial galaxy formation. CIBER consists of a wide-field two-color camera, a low-resolution absolute spectrometer, and a high-resolution narrow-band imaging spectrometer. Currently, all the subsystems have been built, and the integration, testing, and calibration of the CIBER system are on process for the scheduled launch in June 2008.

A Korean team (Korea Astronomy and Space Science Institute, Korea Basic Science Institute, and Kyung Hee University) takes part in an international cooperation project called CIBER (Cosmic Infrared Background ExpeRiment), which has begun with Jet Propulsion Laboratory (JPL) in USA and Institute of Space and Astronautical Science (ISAS) in Japan. CIBER is a rocket-borne instrument, of which the scientific goal is to measure the cosmic near-infrared extra-galactic background to search for signatures of primordial galaxy formation. CIBER consists of a wide-field two-color camera, a low-resolution absolute spectrometer, and a high-resolution narrow-band imaging spectrometer. The Korean team is in charge of the ground support electronics and manufacturing of optical parts of the narrow-band spectrometer, which will provide excellent opportunities for science and technology to Korean infrared groups.

Effects of surface conditions (temperature and roughness) of test specimens, when measuring emissive power of far-infrared ray, have been investigated using FT-IR spectrometer. Element metal zinc (Zn) was selected in this study as representative specimen of materials consisting of simple element. The zinc specimens were heated to four temperatures, i.e., 333K, 353K, .373K, and also their surface was finished with SiC abrasive papers of 100, 220, 360, 400, 600, 800, and 1000 mesh in size. The results shows that the emissive power (W/㎡) of the far-infrared ray increases with temperature for a given roughness and its relationship may be expressed by the following equations: Yη=1.0=0.142.T-0.937 for η=1.0, and Yη=10=0.016.T-1.286 for η=10. The emissive power is also known to increase with surface roughness for a given temperature. Their relationship can be represented by the following equations: YT=313K=0.234.ln(η)+3.53, at 313K, YT=353K=0.234.ln(η)+4.02 at 353K and YT=393K=0.243.ln(η)+4.62 at 393K.