On the disintegration of cosmic ray nuclei by solar photons

We discuss in detail the possibility of observing pairs of simultaneous parallel air showers produced by the fragments of cosmic ray nuclei which disintegrated in collisions with solar photons. We consider scenarios with different cosmic ray compositions, exploring the predicted rates for existing a...

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Autores principales: Epele, Luis Nicolás, Mollerach, Silvia, Roulet, Esteban
Formato: Articulo
Lenguaje:Inglés
Publicado: 1999
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/122780
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id I19-R120-10915-122780
record_format dspace
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
Física
Ciencias Exactas
Cosmic ray
Physics
Astronomy
Photon
Telescope
Angular orientation
PAMELA detector
Astrophysics
Ultra-high-energy cosmic ray
Detector
Plane (geometry)
spellingShingle Ciencias Astronómicas
Física
Ciencias Exactas
Cosmic ray
Physics
Astronomy
Photon
Telescope
Angular orientation
PAMELA detector
Astrophysics
Ultra-high-energy cosmic ray
Detector
Plane (geometry)
Epele, Luis Nicolás
Mollerach, Silvia
Roulet, Esteban
On the disintegration of cosmic ray nuclei by solar photons
topic_facet Ciencias Astronómicas
Física
Ciencias Exactas
Cosmic ray
Physics
Astronomy
Photon
Telescope
Angular orientation
PAMELA detector
Astrophysics
Ultra-high-energy cosmic ray
Detector
Plane (geometry)
description We discuss in detail the possibility of observing pairs of simultaneous parallel air showers produced by the fragments of cosmic ray nuclei which disintegrated in collisions with solar photons. We consider scenarios with different cosmic ray compositions, exploring the predicted rates for existing and planned detectors and looking for methods to extract information on the initial composition from the characteristics of the signal. In particular, we find that fluorescence detectors, such as HiRes or the Telescope Array, due to their low threshold ( ~ 1017 eV) and large area ( ~ 104 km2) may observe several events per year if cosmic rays at those energies are indeed heavy nuclei. The possibility of exploiting the angular orientation of the plane containing the two showers to further constrain the cosmic ray composition is also discussed.
format Articulo
Articulo
author Epele, Luis Nicolás
Mollerach, Silvia
Roulet, Esteban
author_facet Epele, Luis Nicolás
Mollerach, Silvia
Roulet, Esteban
author_sort Epele, Luis Nicolás
title On the disintegration of cosmic ray nuclei by solar photons
title_short On the disintegration of cosmic ray nuclei by solar photons
title_full On the disintegration of cosmic ray nuclei by solar photons
title_fullStr On the disintegration of cosmic ray nuclei by solar photons
title_full_unstemmed On the disintegration of cosmic ray nuclei by solar photons
title_sort on the disintegration of cosmic ray nuclei by solar photons
publishDate 1999
url http://sedici.unlp.edu.ar/handle/10915/122780
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AT mollerachsilvia onthedisintegrationofcosmicraynucleibysolarphotons
AT rouletesteban onthedisintegrationofcosmicraynucleibysolarphotons
bdutipo_str Repositorios
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