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IR Spectrometers01:25

IR Spectrometers

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There are two main infrared (IR) spectrophotometers: dispersive IR spectrometers and Fourier transform infrared (FTIR) spectrometers. In a dispersive IR spectrometer, a beam of infrared radiation produced by a hot wire is divided into two parallel equal-intensity beams using mirrors. One beam passes through the sample, while another is a reference beam. The beams then move through the monochromator, which separates the radiations into a continuous spectrum of different frequencies. The...
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Infrared (IR) Spectroscopy: Overview01:09

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When electromagnetic radiation passes through a material, atoms or molecules transition from a lower to a higher energy state by absorbing radiation corresponding to the energy difference between the two states. The absorption of infrared (IR) radiation causes transitions between vibrational energy levels in a molecule. Therefore, IR spectroscopy is a useful analytical tool for determining the molecular structure of molecules.
Different compounds display unique properties due to their...
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IR Spectrum01:19

IR Spectrum

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When infrared (IR) radiation passes through a molecule, the bonds stretch or bend by absorbing the radiation. This absorption creates the molecule's absorption spectrum, which is the plot of its percentage transmittance versus wavenumber.
Transmittance is defined as the ratio of the radiant power passing through a sample to that from the radiation's source. Multiplying the transmittance by 100 gives the percent transmittance (%T), which varies between 100% (no absorption) and 0%...
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Attenuated Total Reflectance (ATR) Infrared Spectroscopy: Overview01:13

Attenuated Total Reflectance (ATR) Infrared Spectroscopy: Overview

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Attenuated total reflectance (ATR) infrared spectroscopy is a powerful analytical technique used to study the composition of materials. It is widely employed in chemistry, materials science, forensic science, and other fields where sample characterization is required. ATR has several advantages over traditional transmission IR spectroscopy, including the requirement of little to no sample preparation and the ability to analyze a wide range of samples.
The ATR process begins by directing a beam...
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Emission Spectra02:39

Emission Spectra

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When solids, liquids, or condensed gases are heated sufficiently, they radiate some of the excess energy as light. Photons produced in this manner have a range of energies, and thereby produce a continuous spectrum in which an unbroken series of wavelengths is present.
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IR Spectroscopy: Molecular Vibration Overview01:24

IR Spectroscopy: Molecular Vibration Overview

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When Infrared (IR) radiation passes through a covalently bonded molecule, the bonds transition from lower to higher vibrational levels. The fundamental vibrational motions that result in infrared absorption can be classified as stretching or bending vibrations.
Stretching vibrations are vibrational motions that occur along the bond line, changing the bond length or distance between two bonded atoms. They are further distinguished as symmetric or asymmetric. In symmetric stretching, the...
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  1. Home
  2. Mirando A Través De Las Nubes De Júpiter Con Imágenes Espectrales De Radio
  1. Home
  2. Mirando A Través De Las Nubes De Júpiter Con Imágenes Espectrales De Radio

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
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Mirando a través de las nubes de Júpiter con imágenes espectrales de radio

Imke de Pater1, R J Sault2, Bryan Butler3

  • 1Department of Astronomy, 501 Campbell Hall, University of California, Berkeley, CA 94720, USA. Faculty of Aerospace Engineering, Delft University of Technology, 2629 HS Delft, Netherlands. SRON Netherlands Institute for Space Research, 3584 CA Utrecht, Netherlands.

Science (New York, N.Y.)
|June 4, 2016

Ver abstracta en PubMed

Resumen
Este resumen es generado por máquina.

Júpiter también.

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Área de la Ciencia:

  • Ciencias planetarias
  • Ciencias atmosféricas
  • La radioastronomía

Sus antecedentes:

  • La atmósfera de Júpiter por debajo de las nubes visibles sigue siendo en gran parte inexplorada.
  • El amoníaco (NH3) es una fuente primaria de opacidad en la atmósfera superior de Júpiter.

Objetivo del estudio:

  • Mapear las capas profundas de la atmósfera de Júpiter debajo de las nubes visibles.
  • Investigar la actividad dinámica y la composición de estas regiones inexploradas.

Principales métodos:

  • Utilizó el Very Large Array (VLA) para el mapeo de longitudes de onda de radio.
  • Profundizaciones atmosféricas sondeadas hasta aproximadamente 8 bar, ~ 100 km por debajo de las nubes visibles.

Principales resultados:

  • Reveló una atmósfera dinámica activa a presiones por debajo de 2-3 bar.
  • Se identificó un cinturón radioactivo con regiones transparentes (baja concentración de amoníaco) que se extienden por debajo de 8 bar.
  • Observamos una onda ecuatorial que lleva gas de amoníaco a profundidades más bajas.
  • Características de radio correlacionadas con puntos calientes teóricos de 5 micras.

Conclusiones:

  • La atmósfera profunda de Júpiter es dinámicamente activa, con características distintas como un cinturón de radio caliente y una onda ecuatorial.
  • Las observaciones de radio proporcionan una ventana única a las regiones atmosféricas oscurecidas por las nubes.
  • Los hallazgos apoyan las teorías que vinculan las ondas ecuatoriales con los puntos calientes de 5 micrómetros.