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The top documents tagged [line strength]
Education
Classification of stars by Aviral Bajpai
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NOAA Water: Instrument and Data Troy Thornberry, Drew Rollins Ru-Shan Gao, Laurel Watts, Steve Ciciora, Rich McLaughlin, David Fahey NOAA ESRL CSD and
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If a star is very hot, the electrons will be freed from the hydrogen atom. (Ionized) Once they are free, they act like particles and emit a continuous
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Travel
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Is the Sodium Na D line useful? Marcel Bergmann Bo Milvang-Jensen
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Chapter 13 Cont’d – Pressure Effects More curves of growth How does the COG depend on excitation potential, ionization potential, atmospheric parameters
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The Green Bank Telescope a powerful instrument for enhancing ALMA science Unblocked Aperture Low sidelobes gives high dynamic range Resistance to Interference
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Stellar Spectra Ay16 Lecture 2 Feb 5, 2008. The Nearest Star SOHO UV Image
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Why Has Global Warming Paused? Argonne National Laboratory March 22, 2013 William Happer Princeton University
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UNNOFIT inversion V. Bommier, J. Rayrole, M. Martínez González, G. Molodij Paris-Meudon Observatory (France) THEMIS Atelier "Inversion et transfert multidimensionnel",
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Unit 8 Section A Reports on Britain Under the Bombs Background information Text structure analysis Summary of the passage Grammar & Language points Difficult
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A discussion of Radiative Transfer Models Thomas J. Kleespies NOAA/NESDIS
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