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Published byPhilippa Lizbeth Long Modified over 8 years ago
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Spectrogram 2-40 A for varying temperature
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Spectra this is how we find out what everything is made of Vinay Kashyap Smithsonian Astrophysical Observatory or, What is Hosung up to? or,
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SOLAR CHROMOSPHERE He II + Si XI 304 A 70 kK + 1 MK SOHO/EIT
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SOLAR CORONA Fe XV 284 A 2 MK SOHO/EIT
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SOLAR CORONA Fe XII 195A 1.5 MK SOHO/EIT
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SOLAR CORONA Fe IX 171 A 1.2 MK SOHO/EIT
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Wavelength Energy Flux Spectrum Atoms Ions
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Simplified H atom Energy levels Spectral lines
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Line intensity Level population Ion balance Abundance Atomic emissivity DEM
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Continuum Processes Radiative Recombination “free-bound” Bremsstrahlung “free-free”
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Spectrogram 2-40 A for varying temperature
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Summary of coronal structure Fredholm integral of first kind
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“ Dan Rather has never shown a spectrum on the CBS Evening News.” Ed Weiler NASA Associate Director
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