Examples of electromagnetic radiation in the following topics:
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- A black body emits radiation called black body radiation.
- A black body in thermal equilibrium (i.e. at a constant temperature) emits electromagnetic radiation called black body radiation.
- Max Planck, in 1901, accurately described the radiation by assuming that electromagnetic radiation was emitted in discrete packets (or quanta).
- Contrary to the common belief that electromagnetic radiation can take continuous values of energy, Planck introduced a radical concept that electromagnetic radiation was emitted in discrete packets (or quanta) of energy.
- Identify assumption made by Max Planck to describe the electromagnetic radiation emitted by a black body
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- The electromagnetic (EM) spectrum is the range of all possible frequencies of electromagnetic radiation.
- The electromagnetic (EM) spectrum is the range of all possible frequencies of electromagnetic radiation .
- In 1886, the physicist Hertz built an apparatus to generate and detect what are now called radio waves, in an attempt to prove Maxwell's equations and detect such low-frequency electromagnetic radiation.
- However, in 1910, British physicist William Henry Bragg demonstrated that gamma rays are electromagnetic radiation, not particles.
- Generally, electromagnetic radiation is classified by wavelength into radio waves, microwaves, terahertz (or sub-millimeter) radiation, infrared, the visible region humans perceive as light, ultraviolet, X-rays, and gamma rays.
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- Electromagnetic radiation can essentially be described as photon streams.
- Planck theorized that "black bodies" (thermal radiators) and other forms of electromagnetic radiation existed not as spectra, but in discrete, "quantized" form.
- In other words, there were only certain energies an electromagnetic wave could have.
- Momentum is classically defined as the product of mass and velocity and thus would intuitively seem irrelevant to a discussion of electromagnetic radiation, which is both massless and composed of waves.
- Relate energy of an electromagnetic wave with the frequency and wavelength
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- Fluorescence is the emission of light by a substance that has absorbed light or other electromagnetic radiation.
- In most cases, the emitted light has a longer wavelength, and therefore lower energy, than the absorbed radiation.
- However, when the absorbed electromagnetic radiation is intense, it is possible for one electron to absorb two photons; this two-photon absorption can lead to emission of radiation having a shorter wavelength than the absorbed radiation.
- The emitted radiation may also be of the same wavelength as the absorbed radiation, termed "resonance fluorescence".
- Unlike fluorescence, a phosphorescent material does not immediately re-emit the radiation it absorbs.
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- We use different names for electromagnetic waves of different wavelengths: radio waves, microwaves, infrared radiation, visible light, ultraviolet radiation, X-rays, and gamma rays .
- The energy of electromagnetic radiation depends on its wavelength (color) and varies over a wide range; a smaller wavelength (or higher frequency) corresponds to a higher energy.
- All objects absorb and emit electromagnetic radiation.
- Gray objects have a uniform ability to absorb all parts of the electromagnetic spectrum.
- (a) A graph of the spectra of electromagnetic waves emitted from an ideal radiator at three different temperatures.
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- Electromagnetic waves are the combination of electric and magnetic field waves produced by moving charges.
- Electromagnetic radiation, is a form of energy emitted by moving charged particles.
- The creation of all electromagnetic waves begins with a charged particle.
- These and many more such devices use electromagnetic waves to transmit data and signals.
- Electromagnetic waves are a self-propagating transverse wave of oscillating electric and magnetic fields.
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- Infrared (IR) light is electromagnetic radiation with longer wavelengths than those of visible light, extending from the nominal red edge of the visible spectrum at 0.74 micrometers (µm) to 1 mm.
- Infrared radiation is popularly known as "heat radiation," but light and electromagnetic waves of any frequency will heat surfaces that absorb them.
- As stated above, while infrared radiation is commonly referred to as heat radiation, only objects emitting with a certain range of temperatures and emissivities will produce most of their electromagnetic emission in the infrared part of the spectrum.
- This is a plot of Earth's atmospheric transmittance (or opacity) to various wavelengths of electromagnetic radiation.
- The electromagnetic spectrum, showing the major categories of electromagnetic waves.
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- EHF runs the range of frequencies from 30 to 300 gigahertz, above which electromagnetic radiation is considered as far infrared light, also referred to as terahertz radiation.
- Microwaves can also be produced by atoms and molecules—e.g., they are a component of electromagnetic radiation generated by thermal agitation.
- The Cosmic Microwave Background Radiation (CMBR) is microwave radiation that permeates all of space, and its discovery supports the Big Bang theory of the origin of the universe.
- Cosmic background radiation of the Big Bang mapped with increasing resolution.
- The electromagnetic spectrum, showing the major categories of electromagnetic waves.
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- In many languages, X-radiation is called Röntgen radiation, after Wilhelm Röntgen, who is usually credited as its discoverer, and who had named it X-radiation to signify an unknown type of radiation.
- The electromagnetic radiation emitted by X-ray tubes generally has a longer wavelength than the radiation emitted by radioactive nuclei.
- Like all electromagnetic radiation, the properties of X-rays (or gamma rays) depend only on their wavelength and polarization.
- X-rays are part of the electromagnetic spectrum, with wavelengths shorter than those of visible light.
- The electromagnetic spectrum, showing the major categories of electromagnetic waves.
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- It is possible to calculate the radiation field to higher order in $L/(c\tau)$.This is necessary if the dipole moment vanishes, for example.
- where $k\equiv\omega/c$$n=0$ gives the dipole radiation, $n=1$ gives the quadrupole radiation and so on.
- The propagation of electromagnetic waves from a source traveling slower and faster than the speed of light in the medium.