1 / 13

~10 2 /m 2 /secondo

~10 2 /m 2 /secondo. ~1/m 2 /anno. Ginocchio. ~1/km 2 /anno. Caviglia. ~1/km 2 /secolo. Misure indirette. Misure dirette. Sviluppo di un EAS e segnali che arrivano al livello di osservazione. Esperimenti attualmente in corso con partecipazione “torinese”. ARGO-YBJ P. Vallania

phoebe-cooley
Télécharger la présentation

~10 2 /m 2 /secondo

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. ~102/m2/secondo ~1/m2/anno Ginocchio ~1/km2/anno Caviglia ~1/km2/secolo Misure indirette Misuredirette

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

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

  4. The Yangbajing Cosmic Ray Laboratory ARGO Tibet ASγ The ARGO-YBJ experiment Longitude 90° 31’ 50” East Latitude 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. 4300 m above the sea level ~ 600 g/cm2

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

  6. KASCADE-Grande = KArlsruhe Shower Core and Array DEtector + Grande and LOPES Measurements of air showers in the energy range E0 = 100 TeV - 1 EeV

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

  8. The Auger Observatory Area ≈ 3000 km2 Aperture ≈ 7400 km2 sr

  9. Surface Array: 1600 Water Tanks 1.5 km spacing 3000 km2 Fluorescence Detectors: 4 Sites 6 Telescopes per site (180° x 30°) 24 Telescopes total

  10. Esperimenti attualmente in fase di sviluppo con interesse di un gruppo“torinese”. CTA P. Vallania C. Vigorito

  11. Sensitivity goal GLAST Crab E.F(>E) [TeV/cm2s] 10% Crab MAGIC 1% Crab CTA AGN and pulsar physics H.E.S.S. Exploring the cutoff regime in Galactic sources A deep look at the TeV sky

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

  13. 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

More Related