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Summary
| Description |
Italiano: Le bande grigie mostrano le regioni di sensibilità dei tre rivelatori di neutrini solari che sono in grado di ricostruirne l'energia degli eventi. Si noti che Borexino e' potenzialmente in grado di vedere tutti i principali tipi di neutrini solari previsti dai modelli solari, mentre Super-Kamiokande e SNO possono osservare solo una piccola frazione (circa 0.02%) del totale. |
| Date | |
| Source | Own work |
| Author | Francesco Vissani |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 10:54, 12 April 2017 | | 3,000 × 2,250 (1.04 MB) | Francesco Vissani | Cross-wiki upload from it.wikipedia.org |
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