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  • ...stributed objects with emission-line spectra (such as the Sun in [[extreme ultraviolet]]), it results in an image of the object at each wavelength of interest, ov ...
    4 KB (554 words) - 05:17, 24 September 2024
  • ...a McMath Fourier-Transform spectrometer. The observed 2 to 0 lines show an extreme [[hyperfine structure]].<ref name=Orion>{{Cite journal |last1=Jefferts |fir ...
    8 KB (1,064 words) - 12:38, 28 November 2024
  • ...13.6 electron volts, but even so it [[transmittance|transmits]] [[extreme ultraviolet]] and [[soft x-ray]] [[radiation]] from [[extragalactic]] objects to a grea ...
    10 KB (1,475 words) - 15:10, 23 November 2024
  • ...[[ultraviolet]] (UV) radiation by ozone and absorption of solar [[extreme ultraviolet]] (XUV) radiation respectively.<ref>{{Cite web|url=https://scied.ucar.edu/s ...
    9 KB (1,332 words) - 09:54, 27 September 2023
  • ...ctrum,<ref name="Young">The frequencies 458 THz (extreme red) and 727 THz (extreme violet) and other colours apparently have been derived from the wavelengths | extreme violet ...
    19 KB (3,075 words) - 08:14, 3 December 2024
  • ...ter]] CMOS process technology node using a wavelength of 193&nbsp;nm (deep ultraviolet). However, with the [[International Technology Roadmap for Semiconductors|I ...
    13 KB (1,784 words) - 14:32, 14 December 2024
  • ...- or He-rich [[Thermosphere|thermospheres]] heated by the strong [[extreme ultraviolet]] radiation flux of the young Sun.<ref>{{Cite journal |last=Lammer |first=H ...ssure, (4) [[Isothermal process|fixed temperature]], (5) perfect [[extreme ultraviolet]] (XUV) absorption, and that (6) pressure decreases to zero as distance fro ...
    17 KB (2,519 words) - 05:37, 19 December 2024
  • ...for insulators and semiconductors valid throughout radio-waves to extreme ultraviolet spectral range ...
    11 KB (1,271 words) - 11:39, 4 February 2025
  • ...a gas-phase sample are ionized by incident [[Ultraviolet#Vacuum UV|vacuum ultraviolet]] (VUV) radiation. In the ensuing [[Photoelectrochemical processes#Photoion ...ass spectra were recorded as a function of electron energy. Tunable vacuum ultraviolet light sources were used in later setups,<ref>{{cite journal |last1=Stockbau ...
    27 KB (3,599 words) - 15:11, 11 March 2024
  • ...irst7=R. A. |title=Digest. International Electron Devices Meeting |chapter=Extreme scaling with ultra-thin Si channel MOSFETs |date=December 2002 |pages=267–2 ...ans, as of early 2017,{{and then what|date=February 2024}} was to use deep ultraviolet (DUV) immersion lithography initially on this process node (N7FF), and tran ...
    50 KB (6,853 words) - 05:04, 12 January 2025
  • ...fifth-harmonic production in neon and argon, strong-field processes in the ultraviolet, generation of very short wavelengths in BaF<sub>2</sub>, which produced x- * {{cite journal | last=Solem | first=J. C. | year=1988b | title=Extreme states of matter: Could antiprotons be used to power table-top equation of ...
    31 KB (4,025 words) - 18:22, 15 January 2025
  • | align="center" |Hg [[:fr:Ultraviolet|UV]] Line ...certain spectral bands, lenses that are highly transparent in the visible, ultraviolet or infrared, resistance to radiation. ...
    70 KB (10,450 words) - 07:19, 26 February 2025
  • ...siology)|respiration]] in the [[hypolimnion]]. If oxygen depletion becomes extreme, aerobic organisms, like fish, may die, resulting in what is known as a "su ...ed carbon. When this particulate organic carbon interacts with 350&nbsp;nm ultraviolet light, dissolved inorganic carbon is formed, removing even more oxygen from ...
    17 KB (2,413 words) - 09:35, 27 November 2024
  • ...an |first=B. E. |author2=V. A. Lipovetskii |date=1974 |title=Galaxies with ultraviolet continuum V |journal=Astrophysics |volume=8 |issue=2 |pages=89–99 |issn=057 ...|title=Spectral Energy Distribution of Markarian 501: Quiescent State vs. Extreme Outburst|journal=Astrophysical Journal|volume=729|issue=2|pages=2 |date=201 ...
    16 KB (2,295 words) - 01:47, 30 December 2024
  • ...ctive decay]] and produce electromagnetic radiation from [[infrared]] to [[ultraviolet]] wavelengths, generating a [[kilonova]].<ref name="Fujibayashi2020"/>{{rp| ...
    20 KB (2,633 words) - 17:15, 18 July 2024
  • ...r was Alaina Henry, using the [[Cosmic Origins Spectrograph]] and the Near Ultraviolet channel.<ref name=GP_J1219_P13293>{{cite web| title=HST Program 13293| url= ...star formation rates (SFR) derived from the [[GALEX]] observations in the Ultraviolet continuum and in the H alpha emission line for a sample of ~800 luminous co ...
    100 KB (14,565 words) - 21:06, 19 February 2025
  • ...olar system conditions including high solar extreme ultraviolet ([[Extreme ultraviolet|EUV]]) radiation<ref name=":04" /><ref name=":10">{{Cite journal |last1=Héb ...
    42 KB (6,017 words) - 07:26, 3 November 2024
  • ...e was measured experimentally.<ref>{{ cite journal|date=2010|title=Extreme Ultraviolet Frequency Comb Metrology|journal=Phys. Rev. Lett. | volume=105 | issue=6 | ...
    33 KB (4,846 words) - 12:15, 13 January 2025
  • ...[Lawrence Livermore National Lab]] Special Collections|series=Chemistry at Extreme Conditions}}</ref> ...E.|date=9 November 2018|title=Unusually complex phase of dense nitrogen at extreme conditions|journal=Nature Communications|volume=9|issue=1|pages=4717|bibcod ...
    50 KB (7,235 words) - 06:23, 11 October 2024
  • ...ysical model call the [[Big Bang]]. The concept includes an early state of extreme temperature and density; a high precision version of the Big Bang model usi ...articles that form by chance, almost immediately break up again due to the extreme energies.) ...
    113 KB (16,057 words) - 00:06, 28 February 2025
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