Energy level: Difference between revisions

From Glossary of Meteorology
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|Meaning=Any of the possible discrete energies of an atom, molecule, or [[nucleus]].
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|Explanation=According to [[Newtonian mechanics]], the [[energy]] of a body is a continuous [[variable]], but  according to the [[quantum theory]], measured energies of bound states are discrete, some said to  be allowed, others forbidden. We are not aware of this discreteness for macroscopic objects because  of the extreme (relative) smallness of the separation between their energy levels. During transitions  from one energy level to another, quanta of [[radiant energy]] are emitted or absorbed, their [[frequency]]  depending on the difference between energy levels. Emissions of this type are responsible for the  [[aurora borealis]], for example.
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== energy level ==
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<div class="definition"><div class="short_definition">Any of the possible discrete energies of an atom, molecule, or [[nucleus]].</div><br/> <div class="paragraph">According to [[Newtonian mechanics]], the [[energy]] of a body is a continuous [[variable]], but  according to the [[quantum theory]], measured energies of bound states are discrete, some said to  be allowed, others forbidden. We are not aware of this discreteness for macroscopic objects because  of the extreme (relative) smallness of the separation between their energy levels. During transitions  from one energy level to another, quanta of [[radiant energy]] are emitted or absorbed, their [[frequency]]  depending on the difference between energy levels. Emissions of this type are responsible for the  [[aurora borealis]], for example.</div><br/> </div>
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Latest revision as of 06:56, 29 March 2024

Any of the possible discrete energies of an atom, molecule, or nucleus.

According to Newtonian mechanics, the energy of a body is a continuous variable, but according to the quantum theory, measured energies of bound states are discrete, some said to be allowed, others forbidden. We are not aware of this discreteness for macroscopic objects because of the extreme (relative) smallness of the separation between their energy levels. During transitions from one energy level to another, quanta of radiant energy are emitted or absorbed, their frequency depending on the difference between energy levels. Emissions of this type are responsible for the aurora borealis, for example.

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