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angstrom
please note:
- the content below is remote from Wikipedia
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{{Other uses}}{{short description|Unit of length; equals 0.1 nanometre}}- the content below is remote from Wikipedia
- it has been imported raw for GetWiki
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History
(File:Anders à ngström painting.jpg|thumb|Portrait of Anders à ngström)In 1868, Swedish physicist Anders Jonas à ngström created a chart of the spectrum of sunlight, in which he expressed the wavelengths of electromagnetic radiation in the electromagnetic spectrum in multiples of one ten-millionth of a millimetre (or {{val|e=-7|u=mm}}.)BOOK, à ngström, A.J., Recherches sur le spectre solaire, Investigations of the solar spectrum, 1868, W. Schultz, Uppsala, Sweden,weblink fr, The 1869 edition (printed by Ferdinand Dümmler in Berlin) contains sketches of the solar spectrum.WEB, A Brief (Incomplete) History of Light and Spectra,weblink ChemTeam, à ngström's chart and table of wavelengths in the solar spectrum became widely used in solar physics community, which adopted the unit and named it after him.{{citation needed|date=April 2020}} It subsequently spread to the fields of astronomical spectroscopy, atomic spectroscopy, and then to other sciences that deal with atomic-scale structures.Although intended to correspond to {{val|e=-10}} metres, that definition was not accurate enough for spectroscopy work. Until 1960 the metre was defined as the distance between two scratches on a bar of platinum-iridium alloy, kept at the BIPM in Paris in a carefully controlled environment. Reliance on that material standard had led to an early error of about one part in 6000 in the tabulated wavelengths. à ngström took the precaution of having the standard bar he used checked against a standard in Paris, but the metrologist Henri Tresca reported it to be so incorrect that à ngström's corrected results were more in error than the uncorrected ones.BOOK, Brand, John C. D., Lines of Light: Sources of Dispersive Spectroscopy, 1800-1930, 1995, CRC Press, 9782884491631, 47,weblink In 1892â1895, Albert A. Michelson and Jean-René Benoît, working at the BIPM with specially developed equipment, determined that the length of the international metre standard was equal to {{gaps|1|553|163.5}} times the wavelength of the red line of the emission spectrum of electrically excited cadmium vapor.JOURNAL, Michelson, Albert A., Benoît, Jean-René, Détermination expérimentale de la valeur du mètre en longueurs d'ondes lumineuses, Travaux et Mémoires du Bureau International des Poids et Mesures, 1895, 11, 1â85,weblink Experimental determination of the value of the meter in terms of the lengths of light waves, fr, From p. 85, translated: "... the final conclusion of this work is that the fundamental unit of the metric system is represented by the following numbers of wavelengths of three emissions of cadmium, in air at 15 °C and at a pressure of 760 mm: Red emission ⦠1 m = {{gaps|1|553|163,5|λR}} ... It follows that the wavelengths of these emissions, always at 15 °C and at 760 mm, are (averages of three determinations): λR = {{gaps|0,643|847|22|μ}}" (where [1 μ = {{val|1|e=-6|u=m}}]" In 1907, the International Union for Cooperation in Solar Research (which later became the International Astronomical Union) defined the international angstrom as precisely 1/6438.4696 of the wavelength of that line (in dry air at 15 °C (hydrogen scale) and 760 mmHg under a gravity of 9.8067 m/s2).Benoît, Jean-René; Fabry, Charles; and Pérot, Alfred; « Nouvelle Détermination du mètre en longueurs d'ondes lumineuses » ["A New Determination of the Metre in Terms of the Wave-length of Light"], Comptes rendus hebdomadaires des séances de l'Académie des sciences, vol. 144, 21 May 1907, p. 1082-1086This definition was endorsed at the 7th General Conference on Weights and Measures (CGPM) in 1927,{{citation needed|date=April 2020}} but the material definition of the metre was retained until 1960.{{Citation |title=Comptes rendus de la 7{{sup|e}} réunion de la Conférence générale des poids et mesures |language=fr |trans-title=Proceedings of the 7{{sup|th}} meeting of the General conference of weights and measures |year=1927 |place=Paris |publisher=Bureau International des Poids et Mesures |url=https://www.bipm.org/utils/common/pdf/CGPM/CGPM7.pdf#page=87&zoom=auto,-18,777 |pages=85â88|archive-url=https://web.archive.org/web/20181118214334weblink |archive-date=2018-11-18 }} From 1927 to 1960, the angstrom remained a secondary unit of length for use in spectroscopy, defined separately from the metre.{{citation needed|date=November 2021}} In 1960, the metre itself was redefined in spectroscopic terms, which allowed the angstrom to be redefined as being exactly 0.1 nanometres.{{citation needed|date=April 2020}}Although still widely used in physics and chemistry, the angstrom is not a formal part of the International System of Units (SI). The closest SI unit is the nanometre ({{val|e=-9|u=m}}). The International Committee for Weights and Measures officially discouraged its use, and does not even mention it in the 9th edition of the official standard (2019). The angstrom is also not included in the European Union's catalogue of units of measure that may be used within its internal market.WEB,weblink The Council of the European Communities, Council Directive 80/181/EEC of 20 December 1979 on the approximation of the laws of the Member States relating to Unit of measurement and on the repeal of Directive 71/354/EEC, 27 May 2009, 2011-09-23,Angstrom star
After the redefinition of the meter in spectroscopic terms, the Angstrom was formally redefined to be 0.1 nanometers. However, there was briefly thought to be a need for a separate unit of comparable size defined directly in terms of spectroscopy. In 1965, J.A. Bearden defined the Angstrom Star (symbol: Ã *) as 0.202901 times the wavelength of the tungsten- content above as imported from Wikipedia
- "angstrom" does not exist on GetWiki (yet)
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- "angstrom" does not exist on GetWiki (yet)
- time: 7:16am EDT - Sat, May 18 2024
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