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See all on WikipediaSpectral line - Wikipedia
A spectral line is a weaker or stronger region in an otherwise uniform and continuous spectrum. It may result from emission or absorption of light in a narrow frequency range, compared with the nearby frequencies. Spectral lines are often used to identify atoms and molecules. These "fingerprints" can be … See more
Spectral lines are the result of interaction between a quantum system (usually atoms, but sometimes molecules or atomic nuclei) … See more
There are a number of effects which control spectral line shape. A spectral line extends over a tiny spectral band with a nonzero range of frequencies, not a single frequency (i.e., a … See more
Strong spectral lines in the visible part of the electromagnetic spectrum often have a unique Fraunhofer line designation, such as K for a line at … See more
Bands
The phrase "spectral lines", when not qualified, usually refers to lines having wavelengths in the visible band of the full electromagnetic spectrum. Many spectral lines occur at wavelengths outside this range. At shorter … See more• Griem, Hans R. (1997). Principles of Plasma Spectroscopy. Cambridge: University Press. ISBN 0-521-45504-9.
• Griem, … See moreWikipedia text under CC-BY-SA license Spectral lines - BYJU'S
WEBWhat are spectral lines? A spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from the emission or absorption of light in a narrow …
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Spectral line | physics | Britannica
WEBSpectral lines are produced by transitions of electrons within atoms or ions. As the electrons move closer to or farther from the nucleus of an atom (or of an ion), energy in …
5.5: Formation of Spectral Lines - Physics LibreTexts
WEBApr 10, 2022 · Explain how emission line spectra and absorption line spectra are formed; Describe what ions are and how they are formed; Explain how spectral lines and …
Spectral Line | COSMOS - Swinburne
WEBA spectral line is like a fingerprint that can be used to identify the atoms, elements or molecules present in a star, galaxy or cloud of interstellar gas. If we separate the …
5.5 Formation of Spectral Lines - Astronomy 2e - OpenStax
WEBExplain how emission line spectra and absorption line spectra are formed; Describe what ions are and how they are formed; Explain how spectral lines and ionization levels in a …
Chapter 5 Section 5.5: The Formation of Spectral Lines
WEBExplain how spectral lines and ionization levels in a gas can help us determine its temperature. We can use Bohr’s model of the atom to understand how spectral lines are …
Guide to Spectroscopy and Spectral Lines - astrobites
WEBWhen acquiring a spectrum of an astronomical object, astronomers rely upon spectral lines to determine a myriad of physical properties, such as composition, temperature, …
Atomic Spectroscopy - Spectral Lines - NIST
WEBOct 3, 2016 · Spectral Lines: Selection Rules, Intensities, Transition Probabilities, Values, and Line Strengths. Emission Intensities (Transition Probabilities) The total power ε …
Spectral Lines - Encyclopedia.com
WEBA spectral line is light of a single frequency, or wavelength, which is emitted (or absorbed) by an atom when an electron changes its energy level. Because the energy levels of …
6.3: Line Spectra and the Bohr Model - Chemistry LibreTexts
WEBNiels Bohr explained the line spectrum of the hydrogen atom by assuming that the electron moved in circular orbits and that orbits with only certain radii were allowed. Lines in the …
5.5 Formation of Spectral Lines – Astronomy
WEBExplain how spectral lines and ionization levels in a gas can help us determine its temperature. We can use Bohr’s model of the atom to understand how spectral lines are formed.
Chapter 7 Spectral Lines - National Radio Astronomy Observatory
WEBSpectral lines are powerful diagnostics of physical and chemical conditions in astronomical objects. Their rest frequencies identify the specific atoms and molecules …
Spectra and What They Can Tell Us - Imagine the Universe!
WEBNov 20, 2014 · Learn how spectra show the intensity of light over a range of energies and how they can reveal the elements, temperature, density, motion, and other properties of …
Spectral Lines: Types, Elements & Formula - Vaia
WEBModern Physics. Spectral Lines. Imagine climbing a ladder one step at a time. The further away from the ground you get, the more potential energy you'll have. In a way, electrons …
2.6: Lines Spectra- Emission and Absorption Lines
WEBLearning Objectives. You will be able to distinguish between emission and absorption lines in a spectrum. You will know how spectral lines are produced. You will be able to …
Spectral Lines - Northern Arizona University
WEBA spectral line is a dark or bright line in an otherwise uniform and continuous spectrum, resulting from an excess or deficiency of photons in a narrow frequency range, …
Formation of Spectral Lines | Astronomy - Lumen Learning
WEBExplain how spectral lines and ionization levels in a gas can help us determine its temperature. We can use Bohr’s model of the atom to understand how spectral lines …
6.3: Atomic Line Spectra and Niels Bohr - Chemistry LibreTexts
WEBExplain the difference between line spectra for absorption and emission of electrons; Calculate the energy associated with the electron at specified energy state; Calculate …
6.3: Atomic Line Spectra and the Bohr Equation
WEBNiels Bohr explained the line spectrum of the hydrogen atom by assuming that the electron moved in circular orbits and that orbits with only certain radii were allowed. Lines in the …
WEBSpectral lines are highly atom-specific, and can be used to identify the chemical composition of any medium capable of letting light pass through it (typically gas is used). …
5.7: Spectral Lines of Atomic Hydrogen - Chemistry LibreTexts
WEBSep 20, 2022 · Spectral Lines of Hydrogen Bohr's model explains the spectral lines of the hydrogen atomic emission spectrum. While the electron of the atom remains in the …
Spectral Lines - Splitting and Fine structure of spectral lines
WEBDefinition of Spectral Lines. The spectral lines represent the dark or bright line in an apparently uniform and continuous spectrum that results from light emission or …
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