• The Bulletin of The Korean Astronomical Society
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• v.33 no.1
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• pp.46.2-46.2
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• 2008

• The Bulletin of The Korean Astronomical Society
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• v.33 no.1
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• pp.46.1-46.1
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• 2008

• Bulletin of the Korean Space Science Society
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• 1999.09a
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• pp.38-38
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• 1999

• Bulletin of the Korean Space Science Society
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• 2000.10a
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• pp.56-56
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• 2000

• Bulletin of the Korean Space Science Society
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• 2004.04a
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• pp.99-99
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• 2004

We detected and analyzed molecular hydrogen fluorescence in the Taurus Cloud using the Far-ultraviolet Imaging Spectrograph (FIMS) on the STSAT-1 which was launched at SeP. 27 2003. FIMS is optimized for observing diffuse emission lines in the interstellar medium in the wavelength bands of 900-l150 and 1300-1700 angstrom. The Taurus region is a local molecular cloud which is good for studying molecular hydrogen fluorescence emissions. (omitted)

• Proceedings of the Korean Environmental Sciences Society Conference
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• 2017.10a
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• pp.168-168
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• 2017

• Proceedings of the Korean Environmental Sciences Society Conference
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• 2017.10a
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• pp.167-167
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• 2017

• Proceedings of the Korean Environmental Sciences Society Conference
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• 2016.10a
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• pp.222-222
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• 2016

• Proceedings of the Korea Society for Energy Engineering kosee Conference
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• 2006.05a
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• pp.325-330
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• 2006

• Proceedings of the Korean Radioactive Waste Society Conference
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• 2006.06a
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• pp.29-29
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• 2006