Utente:Vale maio/Sandbox3: differenze tra le versioni

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|align="right">|''1964''||[[A. G. Doroshkevich]] e [[Igor Dmitriyevich Novikov]] pubblicano una breve nota, dove menzionano la CMB come fenomeno osservabile<ref>{{cite journal|last=Doroshkevich|first=A. G.|last2=Novikov|first2=I.D.|year=1964|title=Mean Density of Radiation in the Metagalaxy and Certain Problems in Relativistic Cosmology|journal=[[Soviet Physics Doklady]]|volume=9|pages=|doi=|bibcode=1964SPhD....9..111D}}</ref>.

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|align="right">|''1964–65''||[[Arno Penzias]] ande [[Robert Woodrow Wilson]] measuremisurano theuna temperaturetemperatura todi be approximatelycirca 3 K. Robert Dicke, [[P. J. E.James Peebles]], P. G. Roll, ande [[David Todd Wilkinson|D. T. Wilkinson]] interpret thisinterpretano radiationquesta asradiazione acome signatureuna offirma thedel bigBig bangBang.

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|align="right">|''1983''||L'[[Unione Sovietica]] lancia la sonda [[RELIKT-1]] Sovietper CMBlo anisotropystudio experimentdella was launchedCMB.

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|align="right">|''1990''||FIRAS measuresmisura thela blackforma bodydel formcorpo ofnero thedello spettro della CMB spectrumcon withprecisione exquisitemolto precisionalta.

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|align="right">|''Gennaio 1992''||Gli scienziati che hanno analizzato i dati della RELIKT-1 dichiarano la scoperta delle anisotropie al seminario astrofico di Mosca.<ref>{{cite news|last=Zaitsev|first=Y.|date=21 November 2006|title=Nobel Prize In Physics: Russia's Missed Opportunities|url=http://www.bilkent.edu.tr/~crs/russianmissedopport.htm|publisher=[[RIA Novosti]]|accessdate=2008-12-11}}</ref>

|align="right">|''Jan 1992''||Scientists who analyzed data from [[RELIKT-1]] spacecraft report the discovery of anisotropy at the Moscow astrophysical seminar.<ref>

{{cite news|last=Zaitsev|first=Y.|date=21 November 2006|title=Nobel Prize In Physics: Russia's Missed Opportunities|url=http://www.bilkent.edu.tr/~crs/russianmissedopport.htm|publisher=[[RIA Novosti]]|accessdate=2008-12-11}}</ref>

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|align="right">|''Aprile 1992''||Gli scienziati che hanno analizzato i dati del [[COBE]] annunciano la scoperta della temperatura primaria delle anisotropie.<ref>{{cite news|last=Sanders|first=R.|coauthors=Kahn, J.|date=13 October 2006|title=UC Berkeley, LBNL cosmologist George F. Smoot awarded 2006 Nobel Prize in Physics|url=http://www.berkeley.edu/news/media/releases/2006/10/03_nobelph.shtml|publisher=[[UC Berkeley|UC Berkeley News]]|accessdate=2008-12-11}}</ref>

|align="right">|''Apr 1992''||Scientists who analyzed data from [[COBE]] DMR announce the discovery of the primary temperature anisotropy.<ref>

{{cite news|last=Sanders|first=R.|coauthors=Kahn, J.|date=13 October 2006|title=UC Berkeley, LBNL cosmologist George F. Smoot awarded 2006 Nobel Prize in Physics|url=http://www.berkeley.edu/news/media/releases/2006/10/03_nobelph.shtml|publisher=[[UC Berkeley|UC Berkeley News]]|accessdate=2008-12-11}}</ref>

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|align="right">|''1999''||Prime misurazioni delle oscillazioni acustiche nelle anisotropie angolari dello spettro della CMB, dalle sonde [[TOCO]], [[Esperimento BOOMERanG|BOOMERanG]] e [[Millimeter Anisotropy eXperiment IMaging Array|MAXIMA]].

|align="right">|''1999''||First measurements of acoustic oscillations in the CMB anisotropy angular power spectrum from the TOCO, BOOMERANG, and Maxima Experiments.

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|align="right">|''2002''||PolarizationPolarizzazione discoveredscoperta bydalla sonda [[DASI]].<ref>

{{cite journal|last=Kovac|first=J.M.|coauthors=''et al.''|year=2002|title=Detection of polarization in the cosmic microwave background using DASI|journal=[[Nature (journal)|Nature]]|volume=420|issue=6917|pages=772–787|doi=10.1038/nature01269|pmid=12490941}}</ref>

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|align="right">|''2004''||Spettro della polarizzazione E-mode polarization spectrum obtainedottenuto bydalla thesonda [[CBI]].<ref>

{{cite journal|last=Readhead|first=A. C. S.|coauthors=''et al.''|year=2004|title=Polarization Observations with the Cosmic Background Imager|journal=[[Science (journal)|Science]]|volume=306|issue=5697|pages=836–844|doi=10.1126/science.1105598|pmid=15472038}}</ref>

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|align="right">|''2005''||[[Ralph A. Alpher]] isviene awardedinsignito thedella [[National Medal of Science]] forper hisil groundbreakingsuo worklavoro inpionieristico nucleosynthesisnella andnucleosintesi predictione thatla theprevisione universeche expansionl'espansione leavesdell'universo behindlascia backgrounddietro radiationdi sè la radiazione di fondo, thusfornendo providingcosì aun modelmodello forper thela teoria del Big Bang theory.

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|align="right">|''2006''||TwoDue ofdei COBE'sricercatori principalprincipali investigatorsdel [[COBE]], [[George F. Smoot|GeorgeFitzgerald Smoot]] ande [[John C. Mather|JohnCromwell Mather]], receivedricevono theil [[Premio Nobel Prizeper inla Physicsfisica]] in 2006per foril theirloro worklavoro onsule precisionmisure measurementdi ofprecisione thedella CMBRCMB.

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