Natural Gamma Ray Spectrometry - translation to ρωσικά
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  1. Λεξικά
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  3. Natural Gamma Ray Spectrometry

Natural Gamma Ray Spectrometry - translation to ρωσικά

QUANTITATIVE STUDY OF THE ENERGY SPECTRA OF GAMMA-RAY SOURCES
Mrinoe; Gamma ray spectroscopy; Gamma spectrometry; Gamma ray spectrometry; Gamma ray detector; Gamma-ray spectroscopy; Gamma-ray detectors; Gamma-ray detector
  • Germanium gamma spectrum of a radioactive Am-Be-source.
  • Laboratory equipment for determination of γ-radiation spectrum with a scintillation counter. The output from the scintillation counter goes to a Multichannel Analyzer which processes and formats the data.

Natural Gamma Ray Spectrometry      

нефтегазовая промышленность

фирм.аппаратура спектрометрического гамма-каротажа

gamma decay         
  • Gamma emission spectrum of cobalt-60
  • The total absorption coefficient of aluminium (atomic number 13) for gamma rays, plotted versus gamma energy, and the contributions by the three effects. As is usual, the photoelectric effect is largest at low energies, Compton scattering dominates at intermediate energies, and pair production dominates at high energies.
  • Alpha radiation]] consists of [[helium]] nuclei and is readily stopped by a sheet of paper. [[Beta radiation]], consisting of [[electron]]s or [[positron]]s, is stopped by an aluminium plate, but gamma radiation requires shielding by dense material such as lead or concrete.
  • The red dots show some of the ~500 terrestrial gamma-ray flashes daily detected by the Fermi Gamma-ray Space Telescope through 2010. Credit: NASA/Goddard Space Flight Center.
  • 60}}
  • NASA guide to electromagnetic spectrum showing overlap of frequency between X-rays and gamma rays
  • In practice, gamma ray energies overlap with the range of X-rays, especially in the higher-frequency region referred to as "hard" X-rays. This depiction follows the older convention of distinguishing by wavelength.
  • Image of entire sky in 100 MeV or greater gamma rays as seen by the EGRET instrument aboard the [[CGRO]] spacecraft. Bright spots within the galactic plane are [[pulsar]]s while those above and below the plane are thought to be [[quasar]]s.
  • A [[hypernova]]. Artist's illustration showing the life of a [[massive star]] as [[nuclear fusion]] converts lighter elements into heavier ones. When fusion no longer generates enough pressure to counteract gravity, the star rapidly collapses to form a [[black hole]]. Theoretically, energy may be released during the collapse along the axis of rotation to form a long duration [[gamma-ray burst]].
  • access-date=2011-11-08}}</ref>
  • Fermi's]] Large Area Telescope (LAT).
  • The total absorption coefficient of lead (atomic number 82) for gamma rays, plotted versus gamma energy, and the contributions by the three effects. Here, the photoelectric effect dominates at low energy. Above 5 MeV, pair production starts to dominate.
  • VACIS]] (vehicle and container imaging system)
ELECTROMAGNETIC RADIATION OF HIGH FREQUENCY AND THEREFORE HIGH ENERGY
Gamma-ray; Gamma radiation; Gamma Ray; Gamma decay; Gamma particle; Gamma Radiation; Γ Radaition; Gamma particles; Gamma Rays; Gamma photon; Gamma Rays and their characteristics; Gamma-Ray; Gamma-rays; Gammaray; G Radaition; Gamma Ray Control; Gamma rays; Secondary radiation; Gamma-decay; Γ-ray; Γ-rays; Γ radiation; Gamma-ray source; Gamma-ray production; Gamma ray generation; Gamma ray production; Gamma-ray generation; Gamma emission; Γ ray; Y photons; Γ rays; Gamma-irradidated; Gamma-irradiated

[gæmədi'kei]

физика

гамма-распад

gamma-ray source         
  • Gamma emission spectrum of cobalt-60
  • The total absorption coefficient of aluminium (atomic number 13) for gamma rays, plotted versus gamma energy, and the contributions by the three effects. As is usual, the photoelectric effect is largest at low energies, Compton scattering dominates at intermediate energies, and pair production dominates at high energies.
  • Alpha radiation]] consists of [[helium]] nuclei and is readily stopped by a sheet of paper. [[Beta radiation]], consisting of [[electron]]s or [[positron]]s, is stopped by an aluminium plate, but gamma radiation requires shielding by dense material such as lead or concrete.
  • The red dots show some of the ~500 terrestrial gamma-ray flashes daily detected by the Fermi Gamma-ray Space Telescope through 2010. Credit: NASA/Goddard Space Flight Center.
  • 60}}
  • NASA guide to electromagnetic spectrum showing overlap of frequency between X-rays and gamma rays
  • In practice, gamma ray energies overlap with the range of X-rays, especially in the higher-frequency region referred to as "hard" X-rays. This depiction follows the older convention of distinguishing by wavelength.
  • Image of entire sky in 100 MeV or greater gamma rays as seen by the EGRET instrument aboard the [[CGRO]] spacecraft. Bright spots within the galactic plane are [[pulsar]]s while those above and below the plane are thought to be [[quasar]]s.
  • A [[hypernova]]. Artist's illustration showing the life of a [[massive star]] as [[nuclear fusion]] converts lighter elements into heavier ones. When fusion no longer generates enough pressure to counteract gravity, the star rapidly collapses to form a [[black hole]]. Theoretically, energy may be released during the collapse along the axis of rotation to form a long duration [[gamma-ray burst]].
  • access-date=2011-11-08}}</ref>
  • Fermi's]] Large Area Telescope (LAT).
  • The total absorption coefficient of lead (atomic number 82) for gamma rays, plotted versus gamma energy, and the contributions by the three effects. Here, the photoelectric effect dominates at low energy. Above 5 MeV, pair production starts to dominate.
  • VACIS]] (vehicle and container imaging system)
ELECTROMAGNETIC RADIATION OF HIGH FREQUENCY AND THEREFORE HIGH ENERGY
Gamma-ray; Gamma radiation; Gamma Ray; Gamma decay; Gamma particle; Gamma Radiation; Γ Radaition; Gamma particles; Gamma Rays; Gamma photon; Gamma Rays and their characteristics; Gamma-Ray; Gamma-rays; Gammaray; G Radaition; Gamma Ray Control; Gamma rays; Secondary radiation; Gamma-decay; Γ-ray; Γ-rays; Γ radiation; Gamma-ray source; Gamma-ray production; Gamma ray generation; Gamma ray production; Gamma-ray generation; Gamma emission; Γ ray; Y photons; Γ rays; Gamma-irradidated; Gamma-irradiated

физика

гамма-установка

Ορισμός

ГАММА
(? , ?), третья буква греческого алфавита.
---
в музыке - звукоряд - последование всех звуков лада, расположенных от основного тона в восходящем или нисходящем порядке; имеет объем октавы, но может быть продолжена в соседние октавы. См. также Хроматическая гамма.
---
(обозначается ?) , 1) стотысячная доля эрстеда, 1 ? = 10-5 Э. 2) Редко применяемая дольная единица массы, 1 ? = 10-9 кг, чаще называют микрограммом (мкг).
Εμφάνιση περισσότερων ορισμών

Βικιπαίδεια

Gamma spectroscopy

Gamma-ray spectroscopy is the quantitative study of the energy spectra of gamma-ray sources, such as in the nuclear industry, geochemical investigation, and astrophysics.

Most radioactive sources produce gamma rays, which are of various energies and intensities. When these emissions are detected and analyzed with a spectroscopy system, a gamma-ray energy spectrum can be produced.

A detailed analysis of this spectrum is typically used to determine the identity and quantity of gamma emitters present in a gamma source, and is a vital tool in radiometric assay. The gamma spectrum is characteristic of the gamma-emitting nuclides contained in the source, just like in an optical spectrometer, the optical spectrum is characteristic of the material contained in a sample.

https://en.wikipedia.org/wiki/Gamma spectroscopy
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