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Sky Polarization Observatory

From Wikipedia, the free encyclopedia
Sky Polarization Observatory
Alternative namesSPOrtEdit this at Wikidata
Wavelength22, 32, 90 GHz (1.36, 0.94, 0.33 cm)
Decommissioned2005 Edit this on Wikidata
Angular resolution7 degree Edit this on Wikidata
Websitesport.iasfbo.inaf.itEdit this at Wikidata

TheSky Polarization Observatory (SPOrt) was an Italian instrument planned for launch to theInternational Space Station in for a planned 2-year mission beginning in 2007. There it would observe 80% of the sky for theCosmic microwave background radiation in the frequency range from 20 to 100 GHz. Apart from detecting large scale CMB polarization it will also provide maps of Galactic synchrotron emission at lowest frequencies.

The project was headed by Stefano Cortiglioni of the IASF-CNR in Bologna and completely funded by theItalian Space Agency. Due to the project's reliance on theSpace Shuttle, and the setback of theColumbia disaster, timely launch was unlikely. Cortiglioni therefore canceled the project in 2005 to allow his team to seek more promising research avenues.[1]

Instrumentation

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SPOrt[2] carries four feed horns sensitive at 22, 32 and 90 GHz which feed abolometer with a pixel sensitivity of 1.7 μK.

See also

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References

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  1. ^"Archived copy"(PDF). Archived fromthe original(PDF) on 2015-07-01. Retrieved2008-10-27.{{cite web}}: CS1 maint: archived copy as title (link)
  2. ^S. Cortiglioni; B. Negri (2004), "The Sky Polarization Observatory (SPOrt)",New Astronomy,9 (4):297–327,arXiv:astro-ph/0401193,Bibcode:2004NewA....9..297C,doi:10.1016/j.newast.2003.11.004,S2CID 119349964

External links

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Effects
2023 map of the CMB.
2023 map of the CMB.
2023 map of theCMB.
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