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Presentation transcript:

~10 2 /m 2 /secondo ~1/m 2 /anno~1/km 2 /anno~1/km 2 /secoloGinocchio Caviglia Misure diretteMisure indirette

Sviluppo di un EAS e segnali che arrivano al livello di osservazione

Esperimenti attualmente in corso con partecipazione torinese. ARGO-YBJ P. Vallania C. Vigorito S. Vernetto

Longitude 90° East Latitude 30° North 90 Km North from Lhasa (Tibet) An unconventional EAS-array exploiting the full coverage approach at very high altitude to detect small air showers at an energy threshold of a few hundreds of GeV. The ARGO-YBJ experiment Tibet ASγ ARGO The Yangbajing Cosmic Ray Laboratory 4300 m above the sea level ~ 600 g/cm 2

Esperimenti attualmente in corso con partecipazione torinese. KASCADE-Grande M. Bertaina A.Chiavassa C. Morello G.C. Trinchero

Measurements of air showers in the energy range E 0 = 100 TeV - 1 EeV KASCADE-Grande = KArlsruhe Shower Core and Array DEtector + Grande and LOPES

Esperimenti attualmente in corso con partecipazione torinese. AUGER SD M. Aglietta A. Castellina A. Chiavassa C. Morello FD E. Menichetti R. Mussa

The Auger Observatory Area 3000 km 2 Aperture 7400 km 2 sr

Fluorescence Detectors: 4 Sites 6 Telescopes per site (180° x 30°) 24 Telescopes total Fluorescence Detectors: 4 Sites 6 Telescopes per site (180° x 30°) 24 Telescopes total Surface Array: 1600 Water Tanks 1.5 km spacing 3000 km 2 Surface Array: 1600 Water Tanks 1.5 km spacing 3000 km 2

Esperimenti attualmente in fase di sviluppo con interesse di un gruppotorinese. CTA P. Vallania C. Vigorito

Sensitivity goal Crab 10% Crab 1% Crab GLAST MAGIC H.E.S.S. E. F(>E) [TeV/cm 2 s] AGN and pulsar physics Exploring the cutoff regime in Galactic sources A deep look at the TeV sky CTA

Esperimenti attualmente in fase di sviluppo con interesse di un gruppo torinese. JEM-EUSO M. Bertaina P. Galeotti C. Cassardo S. Ferrarese

JEM-EUSO is a new type of observatory that uses the earth's atmosphere as a detector. JEM-EUSO will be on orbit on the International Space Station (ISS). It observes transient luminous phenomena taking place in the earth's atmosphere caused by particles coming from space. The sensor is a super wide-field telescope that detects extreme energy particles with energy above eV. This remote-sensing instrument orbits around the earth every 90 minutes on board of the International Space Station at the altitude of approximately 400km

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