Characteristics and energy dependence of recurrent galactic cosmic-ray flux depressions and of a forbush decrease with LISA Pathfinder

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dc.contributor	Universitat Politècnica de Catalunya. Departament d'Enginyeria Electrònica
dc.contributor.author	Armano, M.
dc.contributor.author	Audley, H.
dc.contributor.author	Baird, J.
dc.contributor.author	Bassan, M.
dc.contributor.author	Benella, S.
dc.contributor.author	Lobo, J.A.
dc.contributor.author	Ramos Castro, Juan José
dc.date	2018-02-16
dc.identifier.citation	Armano, M., Audley, H., Baird, J., Bassan , M., Benella , S., Lobo, J.A, Ramos, J. Characteristics and energy dependence of recurrent galactic cosmic-ray flux depressions and of a forbush decrease with LISA Pathfinder. "Astrophysical journal", 16 Febrer 2018, vol. 854, núm. 2, p. 1-12.
dc.identifier.citation	0004-637X
dc.identifier.citation	10.3847/1538-4357/aaa774
dc.identifier.uri	http://hdl.handle.net/2117/116282
dc.language.iso	eng
dc.relation	http://iopscience.iop.org/article/10.3847/1538-4357/aaa774/meta
dc.rights	info:eu-repo/semantics/openAccess
dc.subject	Àrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject	Astrophysics
dc.subject	Cosmic rays
dc.subject	instrumentation: Interferometers
dc.subject	Interplanetary medium
dc.subject	Solar–terrestrial relations
dc.subject	Sun: heliosphere
dc.subject	Sun: rotation
dc.subject	Astrofísica
dc.title	Characteristics and energy dependence of recurrent galactic cosmic-ray flux depressions and of a forbush decrease with LISA Pathfinder
dc.type	info:eu-repo/semantics/draft
dc.type	info:eu-repo/semantics/article
dc.description.abstract	The final publication is available at IOS Press through http://dx.doi.org/10.3847/1538-4357/aaa774
dc.description.abstract	Galactic cosmic-ray (GCR) energy spectra observed in the inner heliosphere are modulated by the solar activity, the solar polarity and structures of solar and interplanetary origin. A high counting rate particle detector (PD) aboard LISA Pathfinder, meant for subsystems diagnostics, was devoted to the measurement of GCR and solar energetic particle integral fluxes above 70 MeV n-1 up to 6500 counts s-1. PD data were gathered with a sampling time of 15 s. Characteristics and energy dependence of GCR flux recurrent depressions and of a Forbush decrease dated 2016 August 2 are reported here. The capability of interplanetary missions, carrying PDs for instrument performance purposes, in monitoring the passage of interplanetary coronal mass ejections is also discussed.
dc.description.abstract	Peer Reviewed

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