Detection and investigation of delayed extensive air showers with N e > 5 × 106

JETP Letters ◽  
2007 ◽  
Vol 85 (2) ◽  
pp. 101-103 ◽  
Author(s):  
V. I. Yakovlev ◽  
M. I. Vil’danova ◽  
N. G. Vil’danov
Keyword(s):  
Extensive Air Showers ◽  
Air Showers

Radio emission of extensive air showers

2015 ◽  
Vol 185 (7) ◽  
pp. 673-716
Author(s):  
A.D. Filonenko
Keyword(s):  
Radio Emission ◽  
Extensive Air Showers ◽  
Air Showers

Electron excess and electromagnetic induction effect of extensive air showers

2010 ◽  
Vol 16 (3) ◽  
pp. 3-14 ◽  
Author(s):  
V.M. Kartashev ◽  
◽  
P.S. Kizim ◽  
V.E. Kovtun ◽  
S.N. Stervoiedov ◽  
...  
Keyword(s):  
Electromagnetic Induction ◽  
Extensive Air Showers ◽  
Induction Effect ◽  
Air Showers

scholarly journals Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

2021 ◽  
Vol 126 (15) ◽  
Author(s):  
A. Aab ◽  
P. Abreu ◽  
M. Aglietta ◽  
J. M. Albury ◽  
I. Allekotte ◽  
...  
Keyword(s):  
Extensive Air Showers ◽  
Pierre Auger Observatory ◽  
Air Showers

scholarly journals Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

2016 ◽  
Vol 116 (24) ◽  
Author(s):  
A. Aab ◽  
P. Abreu ◽  
M. Aglietta ◽  
E. J. Ahn ◽  
I. Al Samarai ◽  
...  
Keyword(s):  
Radio Signal ◽  
Cosmic Ray ◽  
Radiation Energy ◽  
Extensive Air Showers ◽  
Air Showers

scholarly journals Extensive air showers with TeV-scale quantum gravity

2001 ◽  
Vol 63 (12) ◽  
Author(s):  
Luis Anchordoqui ◽  
Haim Goldberg ◽  
Thomas McCauley ◽  
Thomas Paul ◽  
Stephen Reucroft ◽  
...  
Keyword(s):  
Quantum Gravity ◽  
Extensive Air Showers ◽  
Air Showers

Low-energy muons in extensive air showers at 800 g cm−2

1968 ◽  
Vol 46 (10) ◽  
pp. S131-S135 ◽  
Author(s):  
B. K. Chatterjee ◽  
N. V. Gopalakrishnan ◽  
G. T. Murthy ◽  
S. Naranan ◽  
B. V. Sreekantan ◽  
...  
Keyword(s):  
Size Range ◽  
Low Energy ◽  
Extensive Air Showers ◽  
Air Showers ◽  
Average Total Number ◽  
The Right ◽  
Electron Photon ◽  
Photon Component ◽  
Lateral Structure ◽  
Right Ascension

The following results on the low-energy (> 0.6 GeV and > 1.0 GeV) muons in air showers of size 105 to 2 × 107 at Ootacamund (800 g cm−2) are obtained: (1) The average total number of muons [Formula: see text] varies as Ne0.32 ± 0.2 for 105 < Ne < 106, and as Ne0.8 ± 0.15for 106 < Ne < 2 × 107. (2) In showers showing flat electron lateral structure, the [Formula: see text] variation with Ne is similar to (1). However, in steep showers, [Formula: see text] varies as Ne0.75 ± 0.15 in the whole size range 105 to 2 × 107. (3) "Muon-rich" showers of size < 106 have less energy in the electron–photon component compared to "normal" showers. No such difference is found for showers of size > 106. (4) There is a slight indication of a deficiency of muon-rich showers having a flat lateral distribution of electrons in the right ascension interval 15–21 hours for showers of size 106–107. A similar deficit of showers was observed by the Tokyo group for muon-rich showers in the same RA interval.

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