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EMMA—a new underground cosmic-ray experiment
Authors:T. Enqvist  V. Föhr  J. Joutsenvaara  P. Keränen  P. Kuusiniemi  H. Laitala  M. Lehtola  A. Mattila  J. Narkilahti  S. Nurmenniemi  J. Peltoniemi  H. Remes  T. Räihä  C. Shen  M. Reponen  J. Sarkamo  M. Vaittinen  Z. Zhang  T. Jämsén  L. Ding  Q. Zhu  M. Roos  I. Dzaparova  S. Karpov  A. Kurenya  V. Petkov  A. Yanin  H. Fynbo
Affiliation:1. CUPP, Pyh?salmi, Finland
2. Department of Physics, University of Jyv?skyl?, Finland
3. CUPP, University of Oulu, Finland
4. SGO, University of Oulu, Finland
5. IHEP, Chinese Academy of Sciences, Beijing, China
6. Department of Physical Sciences, University of Helsinki, Finland
7. INR, Russian Academy of Sciences, Moscow, Russia
8. Department of Physics and Astronomy, University of Aarhus, Denmark
Abstract:An experiment observing underground muons originating from cosmic-ray air showers is under preparation in the Pyhäsalmi mine, Finland. The aim is to cover an area of about 200–300 m2, 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 1015–1016 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.
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