Simulation of the isotropic ultra-high energy photons flux in
the solar magnetic field and a comparison with observations
made by the HAWC and Fermi-LAT observatories

D 2024

Simulation of the isotropic ultra-high energy photons flux in the solar magnetic field and a comparison with observations made by the HAWC and Fermi-LAT observatories

ALVAREZ CASTILLO, David E., Piotr HOMOLA, Bożena PONCYLJUSZ, Dariusz GORA, Dhital NIRAJ et. al.

Základní údaje

Originální název

Simulation of the isotropic ultra-high energy photons flux in the solar magnetic field and a comparison with observations made by the HAWC and Fermi-LAT observatories

Autoři

ALVAREZ CASTILLO, David E., Piotr HOMOLA, Bożena PONCYLJUSZ, Dariusz GORA, Dhital NIRAJ, Oleksandr SUSHCHOV, Jarosław STASIELAK, Sławomir STUGLIK, Vahab NAZARI, Cristina OANCEA, Dmitriy BEZNOSKO, Noemi ZABARI, Alok C. GUPTA, Bohdan HNATYK, Alona MOZGOVA, Marcin KASZTELAN, Marcin BIELEWICZ, Peter KOVACS, Bartosz ŁOZOWSKI, Mikhail V. MEDVEDEV, Justyna MISZCZYK, Łukasz BIBRZYCKI, Michał NIEDŹWIECKI, Katarzyna SMELCERZ, Tomasz HACHAJ, Marcin PIEKARCZYK, Maciej PAWLIK, Krzysztof RZECKI, Matías ROSAS, Karel SMOLEK, Manana SVANIDZE, Revaz BERADZE, Arman TURSUNOV (860 Uzbekistán, domácí), Tadeusz WIBIG, Jilberto ZAMORA-SAA, Justyna MĘDRALA, Gabriela OPIŁA, Jerzy PRYGA, Ophir RUIMI a Mario Rodriguez CAHUANTZI

Vydání

Trieste, Italy, Proceedings of Science, od s. "446-1"-"446-8", 8 s. 2024

Nakladatel

Sissa Medialab Srl

Další údaje

Jazyk

angličtina

Typ výsledku

Stať ve sborníku

Obor

10308 Astronomy

Stát vydavatele

Itálie

Utajení

není předmětem státního či obchodního tajemství

Forma vydání

elektronická verze "online"

Odkazy

URL

Organizační jednotka

Fyzikální ústav v Opavě

ISSN

Klíčová slova anglicky

Earth atmosphere; Fermions; Particle beams; Photons; Secondary emission; Tropics;Cosmic rays

Štítky

RIV25

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 5. 3. 2025 14:33, Mgr. Pavlína Jalůvková

Anotace

V originále

In this contribution we study the possibility of the formation of cosmic ray ensembles (CRE) created by the interaction of ultra-high energy (UHE) photons with the magnetic field of the Sun. The lack of observation of those UHE and the difficulties for their identification given the current methodologies motivates this study. We performed simulations using the PRESHOWER program in order to simulate the expected extensive air showers which might be spatially correlated generated upon entering the Earth’s atmosphere. We found characteristic features like very thing and extremely elongates cascades of secondary photons with their corresponding energies spanning the entire cosmic range spectrum. Shower footprints are as large as hundreds of kilometres. An application of this study is the scenario of gamma-ray emission from the vicinity of the Sun as a result of ultra-high energy photon cascading in the solar magnetic field in order to understand recent observations made by the HAWC and Fermi-LAT observatories.

Citovat

ALVAREZ CASTILLO, David E., Piotr HOMOLA, Bożena PONCYLJUSZ, Dariusz GORA, Dhital NIRAJ, Oleksandr SUSHCHOV, Jarosław STASIELAK, Sławomir STUGLIK, Vahab NAZARI, Cristina OANCEA, Dmitriy BEZNOSKO, Noemi ZABARI, Alok C. GUPTA, Bohdan HNATYK, Alona MOZGOVA, Marcin KASZTELAN, Marcin BIELEWICZ, Peter KOVACS, Bartosz ŁOZOWSKI, Mikhail V. MEDVEDEV, Justyna MISZCZYK, Łukasz BIBRZYCKI, Michał NIEDŹWIECKI, Katarzyna SMELCERZ, Tomasz HACHAJ, Marcin PIEKARCZYK, Maciej PAWLIK, Krzysztof RZECKI, Matías ROSAS, Karel SMOLEK, Manana SVANIDZE, Revaz BERADZE, Arman TURSUNOV, Tadeusz WIBIG, Jilberto ZAMORA-SAA, Justyna MĘDRALA, Gabriela OPIŁA, Jerzy PRYGA, Ophir RUIMI a Mario Rodriguez CAHUANTZI. Simulation of the isotropic ultra-high energy photons flux in the solar magnetic field and a comparison with observations made by the HAWC and Fermi-LAT observatories. Online. In Proceedings of Science. Trieste, Italy: Sissa Medialab Srl, 2024, s. "446-1"-"446-8", 8 s. ISSN 1824-8039.

@inproceedings{83785,
   author = {Alvarez Castillo, David E. and Homola, Piotr and Poncyljusz, Bożena and Gora, Dariusz and Niraj, Dhital and Sushchov, Oleksandr and Stasielak, Jarosław and Stuglik, Sławomir and Nazari, Vahab and Oancea, Cristina and Beznosko, Dmitriy and Zabari, Noemi and Gupta, Alok C. and Hnatyk, Bohdan and Mozgova, Alona and Kasztelan, Marcin and Bielewicz, Marcin and Kovacs, Peter and Łozowski, Bartosz and Medvedev, Mikhail V. and Miszczyk, Justyna and Bibrzycki, Łukasz and Niedźwiecki, Michał and Smelcerz, Katarzyna and Hachaj, Tomasz and Piekarczyk, Marcin and Pawlik, Maciej and Rzecki, Krzysztof and Rosas, Matías and Smolek, Karel and Svanidze, Manana and Beradze, Revaz and Tursunov, Arman and Wibig, Tadeusz and ZamoraandSaa, Jilberto and Mędrala, Justyna and Opiła, Gabriela and Pryga, Jerzy and Ruimi, Ophir and Cahuantzi, Mario Rodriguez},
   address = {Trieste, Italy},
   booktitle = {Proceedings of Science},
   keywords = {Earth atmosphere; Fermions; Particle beams; Photons; Secondary emission; Tropics;Cosmic rays},
   howpublished = {elektronická verze "online"},
   language = {eng},
   location = {Trieste, Italy},
   pages = {"446-1"-"446-8"},
   publisher = {Sissa Medialab Srl},
   title = {Simulation of the isotropic ultra-high energy photons flux in the solar magnetic field and a comparison with observations made by the HAWC and Fermi-LAT observatories},
   url = {https://pos.sissa.it/444/446/pdf},
   year = {2024}
}

TY  - CONF
ID  - 83785
AU  - Alvarez Castillo, David E. - Homola, Piotr - Poncyljusz, Bożena - Gora, Dariusz - Niraj, Dhital - Sushchov, Oleksandr - Stasielak, Jarosław - Stuglik, Sławomir - Nazari, Vahab - Oancea, Cristina - Beznosko, Dmitriy - Zabari, Noemi - Gupta, Alok C. - Hnatyk, Bohdan - Mozgova, Alona - Kasztelan, Marcin - Bielewicz, Marcin - Kovacs, Peter - Łozowski, Bartosz - Medvedev, Mikhail V. - Miszczyk, Justyna - Bibrzycki, Łukasz - Niedźwiecki, Michał - Smelcerz, Katarzyna - Hachaj, Tomasz - Piekarczyk, Marcin - Pawlik, Maciej - Rzecki, Krzysztof - Rosas, Matías - Smolek, Karel - Svanidze, Manana - Beradze, Revaz - Tursunov, Arman - Wibig, Tadeusz - Zamora-Saa, Jilberto - Mędrala, Justyna - Opiła, Gabriela - Pryga, Jerzy - Ruimi, Ophir - Cahuantzi, Mario Rodriguez
PY  - 2024
TI  - Simulation of the isotropic ultra-high energy photons flux in the solar magnetic field and a comparison with observations made by the HAWC and Fermi-LAT observatories
PB  - Sissa Medialab Srl
CY  - Trieste, Italy
KW  - Earth atmosphere
KW  - Fermions
KW  - Particle beams
KW  - Photons
KW  - Secondary emission
KW  - Tropics;Cosmic rays
UR  - https://pos.sissa.it/444/446/pdf
N2  - In this contribution we study the possibility of the formation of cosmic ray ensembles (CRE) created by the interaction of ultra-high energy (UHE) photons with the magnetic field of the Sun. The lack of observation of those UHE and the difficulties for their identification given the current methodologies motivates this study. We performed simulations using the PRESHOWER program in order to simulate the expected extensive air showers which might be spatially correlated generated upon entering the Earth’s atmosphere. We found characteristic features like very thing and extremely elongates cascades of secondary photons with their corresponding energies spanning the entire cosmic range spectrum. Shower footprints are as large as hundreds of kilometres. An application of this study is the scenario of gamma-ray emission from the vicinity of the Sun as a result of ultra-high energy photon cascading in the solar magnetic field in order to understand recent observations made by the HAWC and Fermi-LAT observatories.
ER  -

ALVAREZ CASTILLO, David E., Piotr HOMOLA, Bo$\backslash$.zena PONCYLJUSZ, Dariusz GORA, Dhital NIRAJ, Oleksandr SUSHCHOV, Jarosław STASIELAK, Sławomir STUGLIK, Vahab NAZARI, Cristina OANCEA, Dmitriy BEZNOSKO, Noemi ZABARI, Alok C. GUPTA, Bohdan HNATYK, Alona MOZGOVA, Marcin KASZTELAN, Marcin BIELEWICZ, Peter KOVACS, Bartosz ŁOZOWSKI, Mikhail V. MEDVEDEV, Justyna MISZCZYK, Łukasz BIBRZYCKI, Michał NIED$\backslash$'ZWIECKI, Katarzyna SMELCERZ, Tomasz HACHAJ, Marcin PIEKARCZYK, Maciej PAWLIK, Krzysztof RZECKI, Matías ROSAS, Karel SMOLEK, Manana SVANIDZE, Revaz BERADZE, Arman TURSUNOV, Tadeusz WIBIG, Jilberto ZAMORA-SAA, Justyna MĘDRALA, Gabriela OPIŁA, Jerzy PRYGA, Ophir RUIMI a Mario Rodriguez CAHUANTZI. Simulation of the isotropic ultra-high energy photons flux in the solar magnetic field and a comparison with observations made by the HAWC and Fermi-LAT observatories. Online. In \textit{Proceedings of Science}. Trieste, Italy: Sissa Medialab Srl, 2024, s.~''446-1''-''446-8'', 8 s. ISSN~1824-8039.

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