~10 2 /m 2 /secondo ~1/m 2 /anno~1/km 2 /anno~1/km 2 /secologinocchio caviglia misure direttemisure...
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~102/m2/secondo
~1/m2/anno
~1/km2/anno
~1/km2/secolo
Ginocchio
Caviglia
Misure dirette
Misure indirette
Sviluppo di un EAS e segnali che arrivano al livello di osservazione
• Esperimenti attualmente in corso con partecipazione “torinese”.
ARGO-YBJP. VallaniaC. VigoritoS. Vernetto
Longitude 90° 31’ 50” EastLatitude 30° 06’ 38” 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 ASTibet ASγγARGOARGO
The Yangbajing Cosmic Ray Laboratory
4300 m above the sea level ~ 600 g/cm2
• Esperimenti attualmente in corso con partecipazione “torinese”.
KASCADE-GrandeM. BertainaA.ChiavassaC. MorelloG.C. Trinchero
Measurements of air showers in the energy range E0 = 100 TeV - 1 EeV
KASCADE-Grande= KArlsruhe Shower Core and Array DEtector +
Grandeand LOPES
• Esperimenti attualmente in corso con partecipazione “torinese”.
AUGERSDM. AgliettaA. CastellinaA. ChiavassaC. MorelloFDE. MenichettiR. Mussa
The Auger ObservatoryArea ≈ 3000 km2 Aperture ≈ 7400 km2
sr
Fluorescence Detectors:4 Sites6 Telescopes per site (180° x 30°)24 Telescopes total
Fluorescence Detectors:4 Sites6 Telescopes per site (180° x 30°)24 Telescopes total
Surface Array:1600 Water Tanks1.5 km spacing3000 km2
Surface Array:1600 Water Tanks1.5 km spacing3000 km2
• Esperimenti attualmente in fase di sviluppo con interesse di un gruppo“torinese”.
CTAP. VallaniaC. Vigorito
10-14
10-13
10-12
10-11
10 100 1000 104 105
E x
F(>
E)
[TeV
/cm
2s]
E [GeV]
Sensitivity goal
Crab
10% Crab
1% Crab
GLAST
MAGIC
H.E.S.S.
E.F(>E) [TeV/cm2s]
AGN and pulsar physics
Exploring the cutoff regime in
Galactic sourcesA deep look at
the TeV sky
CTA
• Esperimenti attualmente in fase di sviluppo con interesse di un gruppo “torinese”.
JEM-EUSOM. BertainaP. GaleottiC. CassardoS. 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 1019 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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