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http://dbpedia.org/ontology/abstract L'esperimento EBEX (dall'inglese E and B eL'esperimento EBEX (dall'inglese E and B experiment) misurerà la Radiazione cosmica di fondo (CMB) di una parte del cielo durante due voli sub-orbitali (ad alta quota) su pallone aerostatico. È un esperimento per ottenere un'immagine larga e ad altà fedeltà delle anisotropie di polarizzazione della CMB. Usando un telescopio che vola ad una quota di 42000 metri è possibile ridurre l'assorbimento atmosferico al minimo. Questo permette una riduzione dei costi rispetto ad una sonda spaziale, ma viceversa permette di ottenere la mappa di una piccola parte di cielo, al contrario di una missione spaziale, come ad esempio WMAP. Il primo volo è nel 2008 sopra il Nord America per eseguire dei test. Il volo successivo sarà nel 2009 e il pallone sarà lanciato dalla Stazione McMurdo nell'Antartico. Userà un vortice polare per volare attorno al Polo Sud, ritornando dopo due settimane.l Polo Sud, ritornando dopo due settimane. , EBEX (E and B Experiment) は、宇宙背景放射を高高度気球による準周回軌道上で観測する。この実験機は大きく、高解像度の画像を送ってくれる。高度42000mで望遠鏡を使用して大気によるマイクロ波の減衰を最小に抑える。人工衛星を打ち上げる場合に比べて全天の狭い範囲しか走査できないが少ない費用で実現できる。 最初の飛行試験は2008年に北米で実施される予定である。次は2009年、南極のマクマード基地からの放球を予定している。極循環風により南極上空を2週間で周回する , The E and B Experiment (EBEX) will measureThe E and B Experiment (EBEX) will measure the cosmic microwave background radiation of a part of the sky during two sub-orbital (high-altitude) balloon flights. It is an experiment to make large, high-fidelity images of the CMB polarization anisotropies. By using a telescope which flies at over 42,000 metres high, it is possible to reduce the atmospheric absorption of microwaves to a minimum. This allows massive cost reduction compared to a satellite probe, though only a small part of the sky can be scanned and for shorter duration than a typical satellite mission such as WMAP. The first flight was an engineering flight over North America in 2009. For the science flight, EBEX was launched on 29 December 2012, near McMurdo Station in Antarctica. It circled around the South Pole using the polar vortex winds before landing on 24 January 2013 about 400 miles from McMurdo.January 2013 about 400 miles from McMurdo.
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rdfs:comment EBEX (E and B Experiment) は、宇宙背景放射を高高度気球による準周回軌道上で観測する。この実験機は大きく、高解像度の画像を送ってくれる。高度42000mで望遠鏡を使用して大気によるマイクロ波の減衰を最小に抑える。人工衛星を打ち上げる場合に比べて全天の狭い範囲しか走査できないが少ない費用で実現できる。 最初の飛行試験は2008年に北米で実施される予定である。次は2009年、南極のマクマード基地からの放球を予定している。極循環風により南極上空を2週間で周回する , The E and B Experiment (EBEX) will measureThe E and B Experiment (EBEX) will measure the cosmic microwave background radiation of a part of the sky during two sub-orbital (high-altitude) balloon flights. It is an experiment to make large, high-fidelity images of the CMB polarization anisotropies. By using a telescope which flies at over 42,000 metres high, it is possible to reduce the atmospheric absorption of microwaves to a minimum. This allows massive cost reduction compared to a satellite probe, though only a small part of the sky can be scanned and for shorter duration than a typical satellite mission such as WMAP. a typical satellite mission such as WMAP. , L'esperimento EBEX (dall'inglese E and B eL'esperimento EBEX (dall'inglese E and B experiment) misurerà la Radiazione cosmica di fondo (CMB) di una parte del cielo durante due voli sub-orbitali (ad alta quota) su pallone aerostatico. È un esperimento per ottenere un'immagine larga e ad altà fedeltà delle anisotropie di polarizzazione della CMB. Usando un telescopio che vola ad una quota di 42000 metri è possibile ridurre l'assorbimento atmosferico al minimo. Questo permette una riduzione dei costi rispetto ad una sonda spaziale, ma viceversa permette di ottenere la mappa di una piccola parte di cielo, al contrario di una missione spaziale, come ad esempio WMAP.a missione spaziale, come ad esempio WMAP.
rdfs:label The E and B Experiment , EBEX
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