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Each substance has known specific maximum of absorption. Comparing spectra substances can be identified.
Charles R. Cowley has written: 'The theory of stellar spectra' -- subject(s): Spectra, Stars 'An introduction to cosmochemistry' -- subject(s): Astrogeology, Astrophysics, Cosmochemistry 'Line identification studies using traditional techniques and wavelength coincidence statistics' -- subject(s): Abundance, Line spectra, Statistical analysis, Stellar spectra
Has to be greater than .95 to be accurate Spectra corresponds (same) Physical properties match
J. C. McLennan has written: 'Report on some sources of helium in the British empire' -- subject(s): Helium, Gases 'On the radioactivity of mineral oils and natural gases' -- subject(s): Radioactivity, Mineral oils, Gases 'On the absorption spectra of mercury, cadmium, zinc, and other metallic vapours' -- subject(s): Spectra, Mercury, Cadmium, Absorption spectra, Zinc 'The radioactivity of lead' -- subject(s): Radioactivity, Lead 'Electric screening in vacuum tubes' -- subject(s): Experiments, Electric discharges through gases, Electrodes
The color of the light radiated by the spectra can show the internal composition as well as the gases burning on the outer layer. Red stars are colder and blue stars are hotter.
Lothar Frommhold has written: 'Collision-induced absorption in gases' -- subject(s): Absorption and adsorption, Gases, Infrared radiation, Molecular spectra 'Collision-induced Absorption in Gases (Cambridge Monographs on Atomic, Molecular and Chemical Physics)'
The Sun spectra is considered continuous.
There are three main types of infrared spectra: absorption spectra, emission spectra, and reflection spectra. Absorption spectra are produced when a material absorbs infrared energy, emission spectra are produced when a material emits infrared radiation, and reflection spectra result from the reflection of infrared radiation off a material.
Richard H. Tourin has written: 'Spectroscopic gas temperature measurement' -- subject(s): Gases, Plasma spectroscopy, Pyrometry, Spectra
Yes, it is possible to use emission line spectra to determine the presence of metallic ions in the sun. Solids, liquids, and dense gases emit light of all wavelengths, without any gaps. We call this a continuous spectrum
There is no code for spectra
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