6533b851fe1ef96bd12a9648
RESEARCH PRODUCT
EMMA – a new underground cosmic-ray experiment
M. VaittinenZong-xian ZhangTimo EnqvistWladyslaw Henryk TrzaskaJ. NarkilahtiT. JämsénP. KeränenJ. SarkamoT. S. RäihäM. LehtolaIlya UsoskinJari JoutsenvaaraPasi KuusiniemiA. PennanenJ. PeltoniemiA. MattilaC. Shensubject
PhysicsNuclear and High Energy PhysicsMuonLarge Hadron ColliderPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorCosmic rayThreshold energyAtomic and Molecular Physics and OpticsParticle detectorParticle identificationNuclear physicsAir showerHigh Energy Physics::Experimentdescription
An experiment observing underground muons originating from cosmic-ray air showers is under preparation in the Pyhasalmi mine, Finland. The aim is to cover an area of about 200-300 m(2), and the detector setup is capable of measuring the muon multiplicity and their lateral distribution. The detector is placed at a depth of about 85 m (corresponding about 240 m w.e.), which gives a threshold energy of muons of about 45 GeV. The detection of the multimuon events is motivated by partly unknown composition of the primary cosmic rays in the energy region of 10(15)-10(16) eV, i.e., the knee region. In addition, by measuring only the higher energy muons of the air shower, the lowest energy muons being filtered out by the rock overburden, the data is sensitive also to the studies of the upper parts of the air shower. The experiment will be constructed mainly using drift chambers used previously in LEP detectors at CERN, but it can also be expanded using plastic scintillator detectors. The prototype detector is expected to be running in the beginning of 2006, and the full-size detector by the end of 2007.
year | journal | country | edition | language |
---|---|---|---|---|
2008-01-01 | Nuclear Physics B - Proceedings Supplements |