Cosmic Ray Energy Spectrum derived from the Data of EAS Cherenkov Light Arrays in the Tunka Valley

Clicks: 183
ID: 99845
2019
The extensive air shower Cherenkov light array Tunka-133 collected data during 7 winter seasons from 2009 to 2017. From 2175 hours of data taking, we derived the differential energy spectrum of cosmic rays in the energy range 6 · 1015 2 · 1018 eV. The TAIGA-HiSCORE array is in the process of continuous expansion and modernization. Here we present the results obtained with 28 stations of the first HiSCORE stage from 35 clear moonless nights in the winter of 2017-2018. The combined spectrum of two arrays covers a range of 2 · 1014 – 2 · 1018 eV.
Reference Key
v2019cosmicepj Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors V., Prosin;I., Astapov;P., Bezyazeekov;A., Borodin;M., Brückner;N., Budnev;A., Chiavassa;A., Dyachok;O., Fedorov;A., Gafarov;A., Garmash;V., Grebenyuk;O., Gress;T., Gress;O., Grishin;A., Grinyuk;D., Horns;N., Kalmykov;Y., Kazarina;V., Kindin;S., Kiryuhin;P., Kirilenko;R., Kokoulin;K., Kompaniets;E., Korosteleva;V., Kozhin;E., Kravchenko;L., Kuzmichev;A., Lagutin;Yu., Lemeshev;V., Lenok;B., Lubsandorzhiev;N., Lubsandorzhiev;R., Mirgazov;R., Mirzoyan;R., Monkhoev;E., Osipova;A., Pakhorukov;A., Pan;M., Panasyuk;L., Pankov;A., Petrukhin;V., Poleschuk;M., Popescu;E., Popova;A., Porelli;E., Postnikov;V., Ptuskin;A., Pushnin;R., Raikin;E., Rjabov;G., Rubtsov;Y., Sagan;V., Samoliga;Yu., Semeney;A., Sidorenkov;A., Silaev;A., Silaev (junior);A., Skurikhin;M., Slunecka;A., Sokolov;C., Spiering;L., Sveshnikova;V., Tabolenko;B., Tarashansky;L., Tkachev;M., Tluczykont;N., Ushakov;D., Voronin;R., Wischnewski;A., Zagorodnikov;D., Zhurov;V., Zurbanov;I., Yashin;
Journal epj web of conferences
Year 2019
DOI DOI not found
URL
Keywords

Citations

No citations found. To add a citation, contact the admin at info@scimatic.org

No comments yet. Be the first to comment on this article.