EPJ Web of Conferences
Volume 99, 2015ISVHECRI 2014 – 18th International Symposium on Very High Energy Cosmic Ray Interactions
|Number of page(s)||6|
|Section||Highlight Talks 1|
|Published online||04 August 2015|
Primary CR energy spectrum and mass composition by the data of Tunka-133 array
1 Skobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Moscow, Russian Federation
2 Institute of Applied Physics, Irkutsk State University, Irkutsk, Russian Federation
3 University of Turin, Italy
4 Institute fur Experimentalphysik, University of Hamburg, Germany
5 Institute of Nuclear Research, Russian Academy of Sciences, Moscow, Russian Federation
6 DESY Zeuthen, Germany
7 Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Waves Distribution, Russian Academy of Sciences, Moscow, Russian Federation
a e-mail: email@example.com
Published online: 4 August 2015
The Cherenkov light array for the registration of extensive air showers (EAS) Tunka-133 collected data during 5 winter seasons from 2009 to 2014. The differential energy spectrum of all particles and the dependence of the average maximum depth on the energy in the range of 6 ⋅ 1015–1018 eV measured for 1540 hours of observation are presented.
© Owned by the authors, published by EDP Sciences, 2015
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.