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
radio spectroscopy - traducción al ruso
![Opacity of the Earth's atmosphere for different wavelengths of [[electromagnetic radiation]]. The atmosphere blocks some wavelengths but it is mostly transparent for visible light and a wide range of radio waves.](https://commons.wikimedia.org/wiki/Special:FilePath/Atmospheric electromagnetic opacity.svg?width=200 "Opacity of the Earth's atmosphere for different wavelengths of [[electromagnetic radiation]]. The atmosphere blocks some wavelengths but it is mostly transparent for visible light and a wide range of radio waves.")
![With a [[reflection grating]], incident light is separated into several diffraction orders which separate different wavelengths apart (red and blue lines), excepting the 0-th order (black).](https://commons.wikimedia.org/wiki/Special:FilePath/Blazedgrating.jpg?width=200 "With a [[reflection grating]], incident light is separated into several diffraction orders which separate different wavelengths apart (red and blue lines), excepting the 0-th order (black).")
![Optical spectrum of [[Comet Hyakutake]].](https://commons.wikimedia.org/wiki/Special:FilePath/Spectrum of Comet Hyakutake.gif?width=200 "Optical spectrum of [[Comet Hyakutake]].")
[reidiəuspek'trɔskəpi]
физика
радиоспектроскопия
микроволновая спектроскопия
общая лексика
астроспектроскопия
![3D animation of the symmetric stretch-compress mode of the C–H bonds of [[bromomethane]]](https://commons.wikimedia.org/wiki/Special:FilePath/Bromomethane.gif?width=200 "3D animation of the symmetric stretch-compress mode of the C–H bonds of [[bromomethane]]")
![Sample of an IR spec. reading; this one is from [[bromomethane]] (CH<sub>3</sub>Br), showing peaks around 3000, 1300, and 1000 cm<sup>−1</sup> (on the horizontal axis).](https://commons.wikimedia.org/wiki/Special:FilePath/Bromomethane IR spectroscopy.svg?width=200 "Sample of an IR spec. reading; this one is from [[bromomethane]] (CH<sub>3</sub>Br), showing peaks around 3000, 1300, and 1000 cm<sup>−1</sup> (on the horizontal axis).")
![Stretching and bending oscillations]] of the CO<sub>2</sub> carbon dioxide molecule. Upper left: symmetric stretching. Upper right: antisymmetric stretching. Lower line: degenerate pair of bending modes.](https://commons.wikimedia.org/wiki/Special:FilePath/Co2 vibrations.svg?width=200 "Stretching and bending oscillations]] of the CO<sub>2</sub> carbon dioxide molecule. Upper left: symmetric stretching. Upper right: antisymmetric stretching. Lower line: degenerate pair of bending modes.")
![An interferogram from an [[FTIR]] measurement. The horizontal axis is the position of the mirror, and the vertical axis is the amount of light detected. This is the "raw data" which can be [[Fourier transform]]ed to get the actual spectrum.](https://commons.wikimedia.org/wiki/Special:FilePath/FTIR-interferogram.svg?width=200 "An interferogram from an [[FTIR]] measurement. The horizontal axis is the position of the mirror, and the vertical axis is the amount of light detected. This is the \"raw data\" which can be [[Fourier transform]]ed to get the actual spectrum.")
![cm<sup>−1</sup>]].](https://commons.wikimedia.org/wiki/Special:FilePath/IR-spectroscopy-sample.svg?width=200 "cm<sup>−1</sup>]].")
![Schematics of a two-beam absorption spectrometer. A beam of infrared light is produced, passed through an [[interferometer]] (not shown), and then split into two separate beams. One is passed through the sample, the other passed through a reference. The beams are both reflected back towards a detector, however first they pass through a splitter, which quickly alternates which of the two beams enters the detector. The two signals are then compared and a printout is obtained. This "two-beam" setup gives accurate spectra even if the intensity of the light source drifts over time.](https://commons.wikimedia.org/wiki/Special:FilePath/IR spectroscopy apparatus.svg?width=200 "Schematics of a two-beam absorption spectrometer. A beam of infrared light is produced, passed through an [[interferometer]] (not shown), and then split into two separate beams. One is passed through the sample, the other passed through a reference. The beams are both reflected back towards a detector, however first they pass through a splitter, which quickly alternates which of the two beams enters the detector. The two signals are then compared and a printout is obtained. This \"two-beam\" setup gives accurate spectra even if the intensity of the light source drifts over time.")
![US [[Food and Drug Administration]] scientist uses portable near infrared spectroscopy device to detect potentially illegal substances](https://commons.wikimedia.org/wiki/Special:FilePath/Portable Screening Devices (1435) (8225044148).jpg?width=200 "US [[Food and Drug Administration]] scientist uses portable near infrared spectroscopy device to detect potentially illegal substances")
![CaF<sub>2</sub>]].](https://commons.wikimedia.org/wiki/Special:FilePath/SolnIRcell.jpg?width=200 "CaF<sub>2</sub>]].")
общая лексика
инфракрасный спектрометр
Definición
Wikipedia
Astronomical spectroscopy is the study of astronomy using the techniques of spectroscopy to measure the spectrum of electromagnetic radiation, including visible light, ultraviolet, X-ray, infrared and radio waves that radiate from stars and other celestial objects. A stellar spectrum can reveal many properties of stars, such as their chemical composition, temperature, density, mass, distance and luminosity. Spectroscopy can show the velocity of motion towards or away from the observer by measuring the Doppler shift. Spectroscopy is also used to study the physical properties of many other types of celestial objects such as planets, nebulae, galaxies, and active galactic nuclei.
