Traducción y análisis de palabras por inteligencia artificial ChatGPT
En esta página puede obtener un análisis detallado de una palabra o frase, producido utilizando la mejor tecnología de inteligencia artificial hasta la fecha:
- cómo se usa la palabra
- frecuencia de uso
- se utiliza con más frecuencia en el habla oral o escrita
- opciones de traducción
- ejemplos de uso (varias frases con traducción)
- etimología
свечение - traducción al Inglés
![Комета Лавджоя]], проходящая за свечением неба Земли 22 декабря 2011 года.](https://commons.wikimedia.org/wiki/Special:FilePath/Iss030e015472 Edit.jpg?width=200 "Комета Лавджоя]], проходящая за свечением неба Земли 22 декабря 2011 года.")
luminescence, brightness, fluorescence
![An extremely intense pulse of short-wave UV light in a [[flashtube]] produced this blue persistent-phosphorescence in the amorphous, [[fused silica]] envelope, lasting as long as 20 minutes after the 3.5 microsecond flash.](https://commons.wikimedia.org/wiki/Special:FilePath/Fused silica phosphorescence from a 24 million watt flash.jpg?width=200 "An extremely intense pulse of short-wave UV light in a [[flashtube]] produced this blue persistent-phosphorescence in the amorphous, [[fused silica]] envelope, lasting as long as 20 minutes after the 3.5 microsecond flash.")
![[[Jablonski diagram]] of an energy scheme used to explain the difference between fluorescence and phosphorescence. The excitation of molecule A to its singlet excited state (<sup>1</sup>A*) may, after a short time between absorption and emission (fluorescence lifetime), return immediately to ground state, giving off a photon via fluorescence (decay time). However, sustained excitation is followed by intersystem crossing to the triplet state (<sup>3</sup>A) that relaxes to the ground state by phosphorescence with much longer decay times.](https://commons.wikimedia.org/wiki/Special:FilePath/JablonskiSimple.png?width=200 "[[Jablonski diagram]] of an energy scheme used to explain the difference between fluorescence and phosphorescence. The excitation of molecule A to its singlet excited state (<sup>1</sup>A*) may, after a short time between absorption and emission (fluorescence lifetime), return immediately to ground state, giving off a photon via fluorescence (decay time). However, sustained excitation is followed by intersystem crossing to the triplet state (<sup>3</sup>A) that relaxes to the ground state by phosphorescence with much longer decay times.")
![An [[electron microscope]] reveals vacancy defects in a crystalline lattice of [[molybdenum disulfide]]. The missing sulfur atoms leave [[dangling bonds]] between the molybdenum atoms, creating a trap in the empty spaces.](https://commons.wikimedia.org/wiki/Special:FilePath/MoS2 vacancies.jpg?width=200 "An [[electron microscope]] reveals vacancy defects in a crystalline lattice of [[molybdenum disulfide]]. The missing sulfur atoms leave [[dangling bonds]] between the molybdenum atoms, creating a trap in the empty spaces.")
![Phosphorescent, [[europium]]-doped, [[strontium]] silicate-aluminate oxide powder under visible light, fluorescing/phosphorescing under long-wave [[UV light]], and persistently phosphorescing in total darkness](https://commons.wikimedia.org/wiki/Special:FilePath/Phosphorescent.jpg?width=200 "Phosphorescent, [[europium]]-doped, [[strontium]] silicate-aluminate oxide powder under visible light, fluorescing/phosphorescing under long-wave [[UV light]], and persistently phosphorescing in total darkness")
[fɔsfə'res(ə)ns]
общая лексика
фосфоресценция
свечение
фосфоричность
существительное
общая лексика
фосфоресценция
свечение
фосфоресценция, свечение
![Airglow over [[Auvergne, France]]](https://commons.wikimedia.org/wiki/Special:FilePath/Airglow in Auvergne (France) on 13th of August 2015.jpg?width=200 "Airglow over [[Auvergne, France]]")
![IR]]) captured on 3 March 2011.](https://commons.wikimedia.org/wiki/Special:FilePath/Figure 7.png?width=200 "IR]]) captured on 3 March 2011.")
![Two images of the sky over the [[HAARP]] [[Gakona]] facility using the NRL-cooled [[CCD imager]] at 557.7 nm. The field of view is approximately 38°. The left-hand image shows the background star field with the HF transmitter off. The right-hand image was taken 63 seconds later with the HF transmitter on. Structure is evident in the emission region.](https://commons.wikimedia.org/wiki/Special:FilePath/Induced Airglow (HAARP).gif?width=200 "Two images of the sky over the [[HAARP]] [[Gakona]] facility using the NRL-cooled [[CCD imager]] at 557.7 nm. The field of view is approximately 38°. The left-hand image shows the background star field with the HF transmitter off. The right-hand image was taken 63 seconds later with the HF transmitter on. Structure is evident in the emission region.")
![thumb]]](https://commons.wikimedia.org/wiki/Special:FilePath/Airglow in France.jpg?width=200 "thumb]]")
![thumb]]](https://commons.wikimedia.org/wiki/Special:FilePath/Airglow in France (01-21-2023).jpg?width=200 "thumb]]")
 during the night at the 13th August of 2015.jpg?width=200 "Airglow over Auvergne, France.")
['eəgtəu]
общая лексика
свечение неба
(ночное) свечение атмосферы
существительное
специальный термин
(ночное) свечение неба
свечение атмосферы
Definición
; способность излучать свет. Свечение моря. Свечение растений.
Wikipedia
Собственное свече́ние атмосфе́ры — очень слабое излучение света атмосферой планеты. В случае с атмосферой Земли этот оптический феномен приводит к тому, что ночное небо никогда не является полностью тёмным, даже если исключить свет звёзд и рассеянный свет Солнца с дневной стороны.
Свечение неба является в 1000 раз более интенсивным в дневное время, однако изучение феномена дневного свечения атмосферы затруднено из-за того, что оно теряется в ярком свете Солнца.
