Underground cosmic-ray experiment EMMA

被引：3

作者：

Kuusiniemi, P. ^{[1
]}

Bezrukov, L. ^{[2
]}

Enqvist, T. ^{[1
]}

Fynbo, H. ^{[3
]}

Inzhechik, L. ^{[2
,4
]}

Joutsenvaara, J. ^{[1
]}

Kalliokoski, T. ^{[5
]}

Loo, K. ^{[5
]}

Lubsandorzhiev, B. ^{[2
]}

Monto, T. ^{[5
]}

Petkov, V. ^{[2
]}

Raiha, T. ^{[1
]}

Sarkamo, J. ^{[1
]}

Slupecki, M. ^{[1
]}

Trzaska, W. H. ^{[5
]}

Virkajarvi, A. ^{[1
]}

机构：

[1] Univ Oulu, Oulu So Inst, Oulu, Finland

[2] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia

[3] Univ Aarhus, Dept Phys & Astron, DK-8000 Aarhus C, Denmark

[4] Moscow Inst Phys & Technol, Moscow, Russia

[5] Univ Jyvaskyla, Dept Phys, SF-40351 Jyvaskyla, Finland

来源：

23RD EUROPEAN COSMIC RAY SYMPOSIUM (AND 32ND RUSSIAN COSMIC RAY CONFERENCE) | 2013年 / 409卷

基金：

芬兰科学院;

关键词：

D O I：

10.1088/1742-6596/409/1/012067

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

EMMA (Experiment with MultiMuon Array) is a new approach to study the composition of cosmic rays at the knee region (1 - 10 PeV). The array will measure the multiplicity and lateral distribution of the high-energy muon component of an air shower and its arrival direction on an event-by-event basis. The array operates in the Pyhasalmi Mine, Finland, at a depth of 75 metres (or 210 m.w.e) corresponding to the cut-off energy of approximately 50 GeV for vertical muons. The data recording with a partial array has started and preliminary results of the first test runs are presented.

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页数：4

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