Cosmic ray ensembles as signatures of ultra-high energy photons
interacting with the solar magnetic field

J 2022

Cosmic ray ensembles as signatures of ultra-high energy photons interacting with the solar magnetic field

DHITAL, N.; P. HOMOLA; D. ALVAREZ-CASTILLO; D. GORA; K Almeida CHEMINANT et. al.

Basic information

Original name

Cosmic ray ensembles as signatures of ultra-high energy photons interacting with the solar magnetic field

Authors

Edition

Journal of Cosmology and Astroparticle Physics, GB - Spojené království Velké Británie a, 2022, 1475-7516

Other information

Language

English

Type of outcome

Article in a journal

Field of Study

10308 Astronomy

Country of publisher

United Kingdom of Great Britain and Northern Ireland

Confidentiality degree

is not subject to a state or trade secret

References:

URL

Impact factor

Impact factor: 6.300

RIV identification code

RIV/47813059:19630/22:A0000200

Organization unit

Institute of physics in Opava

DOI

https://doi.org/10.1088/1475-7516/2022/03/038

UT WoS

000773220800001

EID Scopus

2-s2.0-85127364812

Keywords in English

cosmic ray experiments; cosmic ray theory; cosmic rays detectors; ultra high energy cosmic rays

Abstract

In the original language

Propagation of ultra-high energy photons in the solar magnetosphere gives rise to cascades comprising thousands of photons. We study the cascade development using Monte Carlo simulations and find that the photons in the cascades are spatially extended over millions of kilometers on the plane distant from the Sun by 1 AU. We estimate the chance of detection considering upper limits from current cosmic rays observatories in order to provide an optimistic estimate rate of 0.002 events per year from a chosen ring-shaped region around the Sun. We compare results from simulations which use two models of the solar magnetic field, and show that although signatures of such cascades are different for the models used, for practical detection purpose in the ground-based detectors, they are similar.

Cite

DHITAL, N.; P. HOMOLA; D. ALVAREZ-CASTILLO; D. GORA; K Almeida CHEMINANT; B. PONCYLJUSZ; J. MEDRALA; G. OPILA; A. BHATT; B. LOZOWSKI; T. BRETZ; L. DEL PERAL; A. R. DUFFY; A. C. GUPTA; B. HNATYK; P. JAGODA; M. KASZTELAN; K. KOPANSKI; P. KOVACS; M. KRUPINSKI; M. MEDVEDEV; V. NAZARI; M. NIEDZWIECKI; D. OSTROGORSKI; M. PIEKARCZYK; M. D. RODRIGUEZ FRIAS; K. RZECKI; K. SMELCERZ; K. SMOLEK; J. STASIELAK; O. SUSHCHOV; T. WIBIG; K. WOZNIAK; J. ZAMORA-SAA; Z. ZIMBORAS and Arman TURSUNOV. Cosmic ray ensembles as signatures of ultra-high energy photons interacting with the solar magnetic field. Journal of Cosmology and Astroparticle Physics. GB - Spojené království Velké Británie a, 2022, vol. 2022, No 3, p. "038-1"-"038-19", 19 pp. ISSN 1475-7516. Available from: https://doi.org/10.1088/1475-7516/2022/03/038.

@article{65444,
   author = {Dhital, N. and Homola, P. and AlvarezandCastillo, D. and Gora, D. and Cheminant, K Almeida and Poncyljusz, B. and Medrala, J. and Opila, G. and Bhatt, A. and Lozowski, B. and Bretz, T. and Del Peral, L. and Duffy, A. R. and Gupta, A. C. and Hnatyk, B. and Jagoda, P. and Kasztelan, M. and Kopanski, K. and Kovacs, P. and Krupinski, M. and Medvedev, M. and Nazari, V. and Niedzwiecki, M. and Ostrogorski, D. and Piekarczyk, M. and Rodriguez Frias, M. D. and Rzecki, K. and Smelcerz, K. and Smolek, K. and Stasielak, J. and Sushchov, O. and Wibig, T. and Wozniak, K. and ZamoraandSaa, J. and Zimboras, Z. and Tursunov, Arman},
   article_location = {GB - Spojené království Velké Británie a},
   article_number = {3},
   doi = {https://doi.org/10.1088/1475-7516/2022/03/038},
   keywords = {cosmic ray experiments; cosmic ray theory; cosmic rays detectors; ultra high energy cosmic rays},
   language = {eng},
   issn = {1475-7516},
   journal = {Journal of Cosmology and Astroparticle Physics},
   title = {Cosmic ray ensembles as signatures of ultra-high energy photons interacting with the solar magnetic field},
   url = {https://iopscience.iop.org/article/10.1088/1475-7516/2022/03/038},
   volume = {2022},
   year = {2022}
}

TY  - JOUR
ID  - 65444
AU  - Dhital, N. - Homola, P. - Alvarez-Castillo, D. - Gora, D. - Cheminant, K Almeida - Poncyljusz, B. - Medrala, J. - Opila, G. - Bhatt, A. - Lozowski, B. - Bretz, T. - Del Peral, L. - Duffy, A. R. - Gupta, A. C. - Hnatyk, B. - Jagoda, P. - Kasztelan, M. - Kopanski, K. - Kovacs, P. - Krupinski, M. - Medvedev, M. - Nazari, V. - Niedzwiecki, M. - Ostrogorski, D. - Piekarczyk, M. - Rodriguez Frias, M. D. - Rzecki, K. - Smelcerz, K. - Smolek, K. - Stasielak, J. - Sushchov, O. - Wibig, T. - Wozniak, K. - Zamora-Saa, J. - Zimboras, Z. - Tursunov, Arman
PY  - 2022
TI  - Cosmic ray ensembles as signatures of ultra-high energy photons interacting with the solar magnetic field
JF  - Journal of Cosmology and Astroparticle Physics
VL  - 2022
IS  - 3
SP  - "038-1"-"038-19"
EP  - "038-1"-"038-19"
SN  - 14757516
KW  - cosmic ray experiments
KW  - cosmic ray theory
KW  - cosmic rays detectors
KW  - ultra high energy cosmic rays
UR  - https://iopscience.iop.org/article/10.1088/1475-7516/2022/03/038
N2  - Propagation of ultra-high energy photons in the solar magnetosphere gives rise to cascades comprising thousands of photons. We study the cascade development using Monte Carlo simulations and find that the photons in the cascades are spatially extended over millions of kilometers on the plane distant from the Sun by 1 AU. We estimate the chance of detection considering upper limits from current cosmic rays observatories in order to provide an optimistic estimate rate of 0.002 events per year from a chosen ring-shaped region around the Sun. We compare results from simulations which use two models of the solar magnetic field, and show that although signatures of such cascades are different for the models used, for practical detection purpose in the ground-based detectors, they are similar.
ER  -

DHITAL, N.; P. HOMOLA; D. ALVAREZ-CASTILLO; D. GORA; K Almeida CHEMINANT; B. PONCYLJUSZ; J. MEDRALA; G. OPILA; A. BHATT; B. LOZOWSKI; T. BRETZ; L. DEL PERAL; A. R. DUFFY; A. C. GUPTA; B. HNATYK; P. JAGODA; M. KASZTELAN; K. KOPANSKI; P. KOVACS; M. KRUPINSKI; M. MEDVEDEV; V. NAZARI; M. NIEDZWIECKI; D. OSTROGORSKI; M. PIEKARCZYK; M. D. RODRIGUEZ FRIAS; K. RZECKI; K. SMELCERZ; K. SMOLEK; J. STASIELAK; O. SUSHCHOV; T. WIBIG; K. WOZNIAK; J. ZAMORA-SAA; Z. ZIMBORAS and Arman TURSUNOV. Cosmic ray ensembles as signatures of ultra-high energy photons interacting with the solar magnetic field. \textit{Journal of Cosmology and Astroparticle Physics}. GB - Spojené království Velké Británie a, 2022, vol.~2022, No~3, p.~''038-1''-''038-19'', 19 pp. ISSN~1475-7516. Available from: https://doi.org/10.1088/1475-7516/2022/03/038.

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