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What is Solar Absorption Spectrum Analysis about?

The document details observations of the solar absorption spectrum and various light sources using analog and digital spectrometers. Key findings include the identification of dark lines in the solar spectrum that correspond to emission lines from hydrogen, as well as some overlap with incandescent lamp spectra. The conclusion suggests that the solar atmosphere is primarily composed of hydrogen, with possible trace amounts of argon and neon.

Author

yuweishi

Language

EN