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Types of Radioactivity03:23

Types of Radioactivity

The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
X-ray Imaging01:24

X-ray Imaging

German physicist Wilhelm Röntgen (1845–1923) was experimenting with electrical current when he discovered that a mysterious and invisible "ray" would pass through his flesh but leave an outline of his bones on a screen coated with a metal compound. In 1895, Röntgen made the first durable record of the internal parts of a living human: an "X-ray" image (as it came to be called) of his wife’s hand. Scientists worldwide quickly began their own experiments with X-rays, and by 1900, X-ray was widely...
The Electromagnetic Spectrum02:37

The Electromagnetic Spectrum

The electromagnetic spectrum consists of all the types of electromagnetic radiation arranged according to their frequency and wavelength. Each of the various colors of visible light has specific frequencies and wavelengths associated with them, and you can see that visible light makes up only a small portion of the electromagnetic spectrum. Because the technologies developed to work in various parts of the electromagnetic spectrum are different, for reasons of convenience and historical...
The Electromagnetic Spectrum01:24

The Electromagnetic Spectrum

Electromagnetic waves are categorized according to their wavelengths and frequencies, giving the electromagnetic spectrum. These waves are classified as radio, infrared, ultraviolet, etc. Radio waves refer to electromagnetic radiation with wavelengths ranging from millimeters to kilometers. Radio waves are commonly used for audio communications (i.e., radios) and typically result from an alternating current in the wires of a broadcast antenna. They cover a broad wavelength range and are used...
IR Frequency Region: X–H Stretching01:24

IR Frequency Region: X–H Stretching

In IR spectroscopy, signals produced by the X−H bonds (such as C−H, O−H, or N−H) can be observed in the frequency range of  2700–4000 cm–1. The C−H stretching vibration forms sharp bands in the region 2850–3000 cm–1. The presence of the O−H stretching vibration leads to the forming of an absorption band in the frequency range 3650–3200 cm−1. At the same time, N−H stretching can be confirmed by absorption bands in the 3500–3100 cm−1 range. Even though both O−H and N−H bonds vibrate at a similar...
Emission Spectra02:39

Emission Spectra

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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Updated: May 19, 2026

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
06:28

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera

Published on: January 30, 2020

ガンマ線が爆発する.

Neil Gehrels1, Péter Mészáros

  • 1Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. neil.gehrels@nasa.gov

Science (New York, N.Y.)
|August 28, 2012
PubMed
まとめ
この要約は機械生成です。

宇宙で最も明るく輝く現象であるガンマ線爆発 (GRB) は,何十年もの研究にもかかわらず,謎のままです. 最近の衛星データは,それらの即時発射と後光についての新しい洞察を提供します.

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Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
06:46

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

Published on: August 25, 2016

関連する実験動画

Last Updated: May 19, 2026

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
06:28

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera

Published on: January 30, 2020

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic
06:46

Applying X-ray Imaging Crystal Spectroscopy for Use as a High Temperature Plasma Diagnostic

Published on: August 25, 2016

科学分野:

  • 天体物理学 天体物理学
  • 宇宙線物理学 宇宙線物理学

背景:

  • ガンマ線爆発 (GRB) は,非常に明るい宇宙の出来事です.
  • 何十年もの研究にもかかわらず,GRBの性質は依然としてほとんど不明である.
  • 先駆的な宇宙と地上の実験は,重要な,しかし不完全なデータを提供しています.

研究 の 目的:

  • スウィフト・衛星とフェルミ・衛星からの最近の観測データをレビューする.
  • 新しいGRB観測と理論モデルの関連性を探求する.
  • 素早く発生するGRBの放出と後発光現象を分析するために.

主な方法:

  • 宇宙ミッションからの最近の観測データを調査する.
  • 経験的データを既存の理論的枠組みと比較する.
  • プロンプトエミッションとアフターグローの特徴を分析する.

主要な成果:

  • スウィフトとフェルミ衛星からの新しいデータは,前例のない洞察を提供します.
  • 観測と理論の相互作用は,GRBを理解するために極めて重要です.
  • プロンプトエミッションとアフターグローの詳細な分析が提示されています.

結論:

  • 最近の進歩は,GRBについての理解を大幅に高めました.
  • 観測データと理論モデリングの継続的な統合は不可欠です.
  • GRBの放出と後発光の謎を完全に解明するには,さらなる研究が必要です.