Solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory

The low energy modes of the surface detector array of the Pierre Auger Observatory record variations in the flux of low energy secondary particles with extreme detail. These two modes consist of recording (1) the rate of signals for energies between 15 MeV and 100 MeV (the Scaler mode) and (2) the c...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autor principal: Masías-Meza, J.J.
Formato: CONF
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_18248039_v30-July-2015_n_p_MasiasMeza
Aporte de:
id todo:paper_18248039_v30-July-2015_n_p_MasiasMeza
record_format dspace
spelling todo:paper_18248039_v30-July-2015_n_p_MasiasMeza2023-10-03T16:33:06Z Solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory Masías-Meza, J.J. The low energy modes of the surface detector array of the Pierre Auger Observatory record variations in the flux of low energy secondary particles with extreme detail. These two modes consist of recording (1) the rate of signals for energies between 15 MeV and 100 MeV (the Scaler mode) and (2) the calibration charge histograms of the individual pulses detected by each water- Cherenkov station, covering different energy channels up to 1 GeV (the Histogram mode). Previous work has studied the flux of galactic cosmic rays on short and intermediate time scales (i.e. from minutes to weeks) using these low energy modes. In this work, after including a longterm correction to the response of the detectors, we present the first long-term analysis of the flux of cosmic rays using scalers and two energy bands of the calibration histograms. We show its sensitivity to the solar cycle variation and its relation to the solar modulation of cosmic rays for an 8-year period. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_18248039_v30-July-2015_n_p_MasiasMeza
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description The low energy modes of the surface detector array of the Pierre Auger Observatory record variations in the flux of low energy secondary particles with extreme detail. These two modes consist of recording (1) the rate of signals for energies between 15 MeV and 100 MeV (the Scaler mode) and (2) the calibration charge histograms of the individual pulses detected by each water- Cherenkov station, covering different energy channels up to 1 GeV (the Histogram mode). Previous work has studied the flux of galactic cosmic rays on short and intermediate time scales (i.e. from minutes to weeks) using these low energy modes. In this work, after including a longterm correction to the response of the detectors, we present the first long-term analysis of the flux of cosmic rays using scalers and two energy bands of the calibration histograms. We show its sensitivity to the solar cycle variation and its relation to the solar modulation of cosmic rays for an 8-year period.
format CONF
author Masías-Meza, J.J.
spellingShingle Masías-Meza, J.J.
Solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory
author_facet Masías-Meza, J.J.
author_sort Masías-Meza, J.J.
title Solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory
title_short Solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory
title_full Solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory
title_fullStr Solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory
title_full_unstemmed Solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory
title_sort solar cycle modulation of cosmic rays observed with the low energy modes of the pierre auger observatory
url http://hdl.handle.net/20.500.12110/paper_18248039_v30-July-2015_n_p_MasiasMeza
work_keys_str_mv AT masiasmezajj solarcyclemodulationofcosmicraysobservedwiththelowenergymodesofthepierreaugerobservatory
_version_ 1807317795027812352