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

File Description SizeFormat 
Armano_2018_ApJ_854_113.pdfPublished version1.38 MBAdobe PDFView/Open
Title: Characteristics and energy dependence of recurrent galactic cosmic-ray Flux depressions and of a Forbush decrease with LISA Pathfinder
Authors: Armano, M
Audley, H
Baird, J
Bassan, M
Benella, S
Binetruy, P
Born, M
Bortoluzzi, D
Cavalleri, A
Cesarini, A
Cruise, AM
Danzmann, K
Silva, MDD
Diepholz, I
Dixon, G
Dolesi, R
Fabi, M
Ferraioli, L
Ferroni, V
Finetti, N
Fitzsimons, ED
Freschi, M
Gesa, L
Gibert, F
Giardini, D
Giusteri, R
Grimani, C
Grzymisch, J
Harrison, I
Heinzel, G
Hewitson, M
Hollington, D
Hoyland, D
Hueller, M
Inchauspe, H
Jennrich, O
Jetzer, P
Karnesis, N
Kaune, B
Korsakova, N
Killow, CJ
Laurenza, M
Lobo, JA
Lloro, I
Liu, L
Lopez-Zaragoza, JP
Maarschalkerweerd, R
Mance, D
Martin, V
Martin-Polo, L
Martino, J
Martin-Porqueras, F
Mateos, I
McNamara, PW
Mendes, J
Mendes, L
Nofrarias, M
Paczkowski, S
Perreur-Lloyd, M
Petiteau, A
Pivato, P
Plagnol, E
Ramos-Castro, J
Reiche, J
Robertson, DI
Rivas, F
Russano, G
Sabbatini, F
Slutsky, J
Sopuerta, CF
Sumner, T
Telloni, D
Texier, D
Thorpe, JI
Vetrugno, D
Vitale, S
Wanner, G
Ward, H
Wass, P
Weber, WJ
Wissel, L
Wittchen, A
Zambotti, A
Zenoni, C
Zweifel, P
Item Type: Journal Article
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.
Issue Date: 16-Feb-2018
Date of Acceptance: 12-Jan-2018
ISSN: 0004-637X
Publisher: American Astronomical Society
Journal / Book Title: Astrophysical Journal
Volume: 854
Issue: 2
Copyright Statement: © 2018. The American Astronomical Society. All rights reserved.
Keywords: Science & Technology
Physical Sciences
Astronomy & Astrophysics
cosmic rays
instrumentation: interferometers
interplanetary medium
solar-terrestrial relations
Sun: heliosphere
Sun: rotation
0201 Astronomical And Space Sciences
0305 Organic Chemistry
0306 Physical Chemistry (Incl. Structural)
Publication Status: Published
Open Access location:
Article Number: ARTN 113
Appears in Collections:Physics
High Energy Physics

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

Creative Commons