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- ...bremsstrahlung]]. It can also be applied in the context of [[gravitational radiation]], and more recently to other field theories by [[Carl Friedrich von Weizsä ==Background== ...5 KB (708 words) - 05:59, 21 January 2024
- The '''radiation law''' is way of modeling human mobility ([[geographic mobility]], [[human ==The radiation model<ref name=simini/>== ...7 KB (1,102 words) - 09:09, 24 November 2024
- ...[Sunlight|solar radiation]] and partially absorbing of [[Infrared|infrared radiation]] from the planet. It provides an approximation for the temperature of the == Background == ...9 KB (1,332 words) - 09:54, 27 September 2023
- ...derived for an accelerating [[magnetic moment]] emitting [[electromagnetic radiation]]. ...ions must be met in order to derive the following formula for the magnetic radiation reaction force. First, the motion of the [[magnetic moment]] must be period ...12 KB (1,849 words) - 02:32, 14 October 2023
- {{Short description|Dose measurement of radiation}} ...equivalent dose''' (FED) is an informal unit of measurement of [[ionizing radiation]] exposure. Expressed in units of flight-time (i.e., flight-seconds, flight ...15 KB (1,865 words) - 14:48, 1 February 2025
- ...ents can be far more chemically reactive than the original molecule, as in radiation therapy for cancer, and are thus a useful field of inquiry. Different '''mo ==Background== ...4 KB (581 words) - 17:56, 4 July 2024
- | known_for = [[Transition radiation detector|Transition Radiation Detectors]] ...Later she started to work with [[Transition radiation detector|Transition Radiation Detector]] prototypes, which were rather new at this time and which require ...8 KB (1,073 words) - 13:19, 9 November 2024
- ...yield the new signal and background. The difference of the new signal and background data is taken to yield the net signal. Finally, the net signal is plotted v ...rget.jpg|thumb|right|250px|Half moon target – on the left the image of the background region and on the right an image of the signal region. Using specialized so ...4 KB (634 words) - 05:53, 22 May 2021
- ...fference in the temperature of neutral hydrogen and the [[cosmic microwave background]] at the end of the [[Timeline of the Big Bang#Dark Ages|Dark Ages]] and th ==Background== ...7 KB (978 words) - 17:50, 12 November 2024
- ...Economic Time Series''). It is a generalization of the [[Planck's law]] of radiation from [[statistical physics]]. ==Background== ...3 KB (461 words) - 20:22, 19 November 2019
- ...stronger K-alpha 1 peak, and the weaker K-alpha 2 peak. Compared to other radiation such as the [[Bremsstrahlung]], the K-alpha two peak is more difficult to f For diffraction experiments with X-rays radiation is usually used with the <math>K_\alpha</math> Wavelength of the anode mate ...5 KB (826 words) - 17:09, 23 April 2024
- ...t an accelerated charge should radiate [[electromagnetic waves]], yet such radiation is not observed for stationary particles in gravitational fields. ...Fulton|first1=Thomas|last2=Rohrlich|first2=Fritz|date=1960|title=Classical radiation from a uniformly accelerated charge|journal=Annals of Physics|volume=9|issu ...15 KB (2,369 words) - 22:30, 25 November 2024
- ...ort description|Astronomical observatory for studying the cosmic microwave background (2008–2010)}} ...xperiment]] to study the polarization of the [[cosmic microwave background radiation]].<ref name="quiet_homepage" /> QUIET stands for '''Q/U Imaging ExperimenT' ...8 KB (1,156 words) - 12:45, 12 February 2025
- ...pectrum. The [[photoemission]] experiment is conducted using [[synchrotron radiation]] light source with typical photon energy of 20 – 100 eV. [[Synchrotron]] l ===Background=== ...11 KB (1,508 words) - 02:12, 24 April 2021
- ..., around 377,000 years after the Big Bang. They form the [[cosmic neutrino background]] (abbreviated CνB or CNB). The neutrinos from this event have a very low e ...verse. At this point in cosmic history, the energy density is dominated by radiation, so that <math>\rho \propto T^4</math>. As the rate of weak interaction dep ...11 KB (1,538 words) - 00:57, 28 August 2021
- ...shielding, reducing [[Cosmic ray|cosmic radiation]] [[Background radiation|background]]. The GERDA experiment was operated from 2011 onwards at LNGS.<ref name="g ...o the expectation that further background reduction was in reach so that a background-free experiment with an even larger source strength, respectively exposure, ...9 KB (1,268 words) - 20:34, 12 February 2023
- ...an experiment to a specific particle interaction, reducing conflation with background interactions by creating more degrees of freedom by which the particle in q ...ed in coincidence, the harder it is to justify such an event occurred from background flux and the higher the experiment's efficiency. As an example, the [[Cowan ...14 KB (1,917 words) - 18:46, 6 August 2024
- ...edium]] in local [[thermodynamic equilibrium]] that both absorbs and emits radiation. ...ar|dI<sub>λ</sub>}}, [W/sr/m<sup>2</sup>/μm]) at a given [[wavelength]] as radiation travels an incremental distance ({{mvar|ds}}) through a non-[[optical scatt ...29 KB (4,329 words) - 05:16, 7 September 2024
- ...a transfer function which mediates the transition from the universe being radiation dominated to being matter dominated. ...irst2=Naoshi | last3=Silk | first3=Joseph | title=The physics of microwave background anisotropies | journal=Nature | publisher=Springer Science and Business Med ...8 KB (1,162 words) - 13:59, 14 April 2024
- ...volving from a Nonsingular Initially De-Sitter Cosmology and the Microwave Background Anisotropy |journal=Sov. Astron. Lett. |volume=9 |pages=302 |year=1983 |las ...these are compatible with experimental data, with 2018 [[cosmic microwave background|CMB]] data from the [[Planck (spacecraft)|Planck satellite]] giving a const ...8 KB (1,085 words) - 04:36, 2 December 2024