Study of composition of cosmic rays with energy .7 E 3 Ee

Learning the Composition of Ultra High Energy Cosmic Rays

Bortolato, Blaz
Kamenik, Jernej F.
Tammaro, Michele

December 2022

We apply statistical inference on the Pierre Auger Open Data to discern for the first time the full ...

The Mass Composition of Ultra-high Energy Cosmic Rays Measured by New Fluorescence Detectors in the Telescope Array Experiment

Fujii, Toshihiro

December 2015

AbstractThe longitudinal development of an extensive air shower reaches its maximum at a depth, Xmax...

Measuring the energy spectrum of primary cosmic rays with the Yakutsk EAS array

Khristiansen, G. B.

February 1986

The Yakutsk Extensive Air Showers (EAS) array was designed for detecting the showers generated by th...

Fluctuations of development maximum depth and nuclear composition of primary cosmic radiation

Dyakonov, M. N.
Struchkov, G. G.
Knurenko, S. P.
Ivanov, A. A.
Pavlov, V. N.
Kolosov, V. A.
Sleptsov, I. Y.
Krasilnikov, D. D.

August 1985

The extensive air showers (EAS) cascade curves from the Cerenkov light lateral distribution measurem...

A Comparative Study of the Depth of Maximum of Simulated Air Shower Longitudinal Profiles

Pryke, C L

January 2001

A comparative study of simulated air shower longitudinal profiles is presented. An appropriate thinn...

MEASUREMENTS OF COSMIC-RAY AIR SHOWER DEVELOPMENT AT ENERGIES ABOVE 1017 eV

G. L. Cassiday
R. Cooper
S. C. Corbato
B. R. Dawson
J. W. Elbert
B. E. Fick
K. D. Green
D. B. Kieda
S. Ko
D. F. Liebing
E. C. Loh
M. H. Salamon
J. D. Smith
P. Sokolsky
P. Sommers
S. B. Thomas
S. X. Wang
B. Wheeler

January 1989

We present measurements of the depth of maximum for extensive air showers (EAS) produced by cosmic r...

Study of cosmic rays above 0.3 EeV using Fly’s Eye‐muon array coincidence

Green, K. D.

April 1991

The Fly’s Eye (FE) and the Michigan Muon Array (MA) simultaneously detect Extensive Air Showers (EAS...

Energy calibration of the fly's eye detector

Sokolsky, P.
Cooper, R.
Baltrusaitis, R. M.
Loh, E. C.
Elbert, J. W.
Ko, S.
Gerhardy, P. R.
Cassiday, G. L.
Mizumoto, Y.
Steck, D.

August 1985

The methods used to calibrate the Fly's eye detector to evaluate the energy of EAS are discussed. Th...

Cosmic-ray composition around 10^18 eV

Kieda, David B.
Stanev, Todor

March 1993

Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...

The lateral distribution of Cerenkov light in large cosmic ray showers as a measure of longitudinal development

Craig, M.A.B

January 1984

This thesis reports measurements made on the longitudinal cascade of high energy cosmic ray showers ...

The lateral distribution of Cerenkov light from extensive air showers

Dawson, Bruce Robert

January 1985

Investigations of the cosmic ray flux around the " knee " in the all - particle energy spectrum can ...

Proton-air inelastic cross section at S(1/2) = 30 TeV

Loh, E. C.
Ko, S.
Cooper, R.
Baltrusaitis, R. M.
Mizumoto, Y.
Cassiday, G. L.
Gerhardy, P. R.
Steck, D.
Elbert, J. W.
Sokolsky, P.

August 1985

The distribution of the maxima of high energy cosmic ray induced extensive air showers in the atmosp...

A Likelihood Method for Measuring the Ultrahigh Energy Cosmic Ray Composition

Abbasi, R U
Abu-Zayyad, T
Amman, J F
Archbold, G C
Belov, K
Blake, S A
Belz, J W
Ben Zvi, S
Bergman, D R
Boyer, J H
Burt, G W
Cao, Z
Connolly, B M
Deng, W
Fedorova, Y
Findlay, J
Finley, C B
Hanlon, W F
Hoffman, C M
Holzscheiter, M H
Hughes, G A
Hüntemeyer, P
Jui, C C H
Kim, K
Kirn, M A
Knapp, B C
Loh, E C
Maestas, M M
Manago, N
Mannel, E J
Marek, L J
Martens, K
Matthews, J A J
Matthews, J N
O'Neill, A
Painter, C A
Perera, L
Reil, K
Riehle, R
Roberts, M
Rodríguez, D
Sasaki, M
Schnetzer, S
Seman, M
Sinnis, G
Smith, J D
Snow, R
Sokolsky, P
Springer, R W
Stokes, B T
Thomas, J R
Thomas, S B
Thomson, G B
Tupa, D
Westerhoff, S
Wiencke, L R

April 2006

Air fluorescence detectors traditionally determine the dominant chemical composit ion of the ultrahi...

Composition of UHE Cosmic Ray Primaries

Poirier, J
Carpenter, J
Gress, J
Lin, T F
Rösch, A

May 2000

Project GRAND presents results on the atomic composition of primary cosmic rays. This is accomplishe...

Monte Carlo simulation of EAS generated by 10(14) - 10(16) eV protons

Stanev, T.
Fenyves, E. J.
Yunn, B. C.

August 1985

Detailed Monte Carlo simulations of extensive air showers to be detected by the Homestake Surface Un...

Learning the Composition of Ultra High Energy Cosmic Rays

Bortolato, Blaz
Kamenik, Jernej F.
Tammaro, Michele

December 2022

We apply statistical inference on the Pierre Auger Open Data to discern for the first time the full ...

The Mass Composition of Ultra-high Energy Cosmic Rays Measured by New Fluorescence Detectors in the Telescope Array Experiment

Fujii, Toshihiro

December 2015

AbstractThe longitudinal development of an extensive air shower reaches its maximum at a depth, Xmax...

Measuring the energy spectrum of primary cosmic rays with the Yakutsk EAS array

Khristiansen, G. B.

February 1986

The Yakutsk Extensive Air Showers (EAS) array was designed for detecting the showers generated by th...

Fluctuations of development maximum depth and nuclear composition of primary cosmic radiation

Dyakonov, M. N.
Struchkov, G. G.
Knurenko, S. P.
Ivanov, A. A.
Pavlov, V. N.
Kolosov, V. A.
Sleptsov, I. Y.
Krasilnikov, D. D.

August 1985

The extensive air showers (EAS) cascade curves from the Cerenkov light lateral distribution measurem...

A Comparative Study of the Depth of Maximum of Simulated Air Shower Longitudinal Profiles

Pryke, C L

January 2001

A comparative study of simulated air shower longitudinal profiles is presented. An appropriate thinn...

MEASUREMENTS OF COSMIC-RAY AIR SHOWER DEVELOPMENT AT ENERGIES ABOVE 1017 eV

G. L. Cassiday
R. Cooper
S. C. Corbato
B. R. Dawson
J. W. Elbert
B. E. Fick
K. D. Green
D. B. Kieda
S. Ko
D. F. Liebing
E. C. Loh
M. H. Salamon
J. D. Smith
P. Sokolsky
P. Sommers
S. B. Thomas
S. X. Wang
B. Wheeler

January 1989

We present measurements of the depth of maximum for extensive air showers (EAS) produced by cosmic r...

Study of cosmic rays above 0.3 EeV using Fly’s Eye‐muon array coincidence

Green, K. D.

April 1991

The Fly’s Eye (FE) and the Michigan Muon Array (MA) simultaneously detect Extensive Air Showers (EAS...

Energy calibration of the fly's eye detector

Sokolsky, P.
Cooper, R.
Baltrusaitis, R. M.
Loh, E. C.
Elbert, J. W.
Ko, S.
Gerhardy, P. R.
Cassiday, G. L.
Mizumoto, Y.
Steck, D.

August 1985

The methods used to calibrate the Fly's eye detector to evaluate the energy of EAS are discussed. Th...

Cosmic-ray composition around 10^18 eV

Kieda, David B.
Stanev, Todor

March 1993

Journal ArticleWe use the depth of maximum distribution as measured by the stereo Fly's Eye detector...

The lateral distribution of Cerenkov light in large cosmic ray showers as a measure of longitudinal development

Craig, M.A.B

January 1984

This thesis reports measurements made on the longitudinal cascade of high energy cosmic ray showers ...

The lateral distribution of Cerenkov light from extensive air showers

Dawson, Bruce Robert

January 1985

Investigations of the cosmic ray flux around the " knee " in the all - particle energy spectrum can ...

Proton-air inelastic cross section at S(1/2) = 30 TeV

Loh, E. C.
Ko, S.
Cooper, R.
Baltrusaitis, R. M.
Mizumoto, Y.
Cassiday, G. L.
Gerhardy, P. R.
Steck, D.
Elbert, J. W.
Sokolsky, P.

August 1985

The distribution of the maxima of high energy cosmic ray induced extensive air showers in the atmosp...

A Likelihood Method for Measuring the Ultrahigh Energy Cosmic Ray Composition

Abbasi, R U
Abu-Zayyad, T
Amman, J F
Archbold, G C
Belov, K
Blake, S A
Belz, J W
Ben Zvi, S
Bergman, D R
Boyer, J H
Burt, G W
Cao, Z
Connolly, B M
Deng, W
Fedorova, Y
Findlay, J
Finley, C B
Hanlon, W F
Hoffman, C M
Holzscheiter, M H
Hughes, G A
Hüntemeyer, P
Jui, C C H
Kim, K
Kirn, M A
Knapp, B C
Loh, E C
Maestas, M M
Manago, N
Mannel, E J
Marek, L J
Martens, K
Matthews, J A J
Matthews, J N
O'Neill, A
Painter, C A
Perera, L
Reil, K
Riehle, R
Roberts, M
Rodríguez, D
Sasaki, M
Schnetzer, S
Seman, M
Sinnis, G
Smith, J D
Snow, R
Sokolsky, P
Springer, R W
Stokes, B T
Thomas, J R
Thomas, S B
Thomson, G B
Tupa, D
Westerhoff, S
Wiencke, L R

April 2006

Air fluorescence detectors traditionally determine the dominant chemical composit ion of the ultrahi...

Composition of UHE Cosmic Ray Primaries

Poirier, J
Carpenter, J
Gress, J
Lin, T F
Rösch, A

May 2000

Project GRAND presents results on the atomic composition of primary cosmic rays. This is accomplishe...

Monte Carlo simulation of EAS generated by 10(14) - 10(16) eV protons

Stanev, T.
Fenyves, E. J.
Yunn, B. C.

August 1985

Detailed Monte Carlo simulations of extensive air showers to be detected by the Homestake Surface Un...

Learning the Composition of Ultra High Energy Cosmic Rays

Bortolato, Blaz
Kamenik, Jernej F.
Tammaro, Michele

December 2022

We apply statistical inference on the Pierre Auger Open Data to discern for the first time the full ...

The Mass Composition of Ultra-high Energy Cosmic Rays Measured by New Fluorescence Detectors in the Telescope Array Experiment

Fujii, Toshihiro

December 2015

AbstractThe longitudinal development of an extensive air shower reaches its maximum at a depth, Xmax...

Measuring the energy spectrum of primary cosmic rays with the Yakutsk EAS array

Khristiansen, G. B.

February 1986

The Yakutsk Extensive Air Showers (EAS) array was designed for detecting the showers generated by th...

Study of composition of cosmic rays with energy .7 E 3 Ee

Abstract

Extracted data

Study of composition of cosmic rays with energy .7 E 3 Ee

Abstract

Extracted data

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