Imperial College London

ProfessorTimothySumner

Faculty of Natural SciencesDepartment of Physics

Professor of Experimental Astrophysics
 
 
 
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Contact

 

+44 (0)20 7594 7552t.sumner

 
 
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Location

 

1108Blackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@article{Armano:2018:1538-4357/aaa774,
author = {Armano, M and Audley, H and Baird, J and Bassan, M and Benella, S and Binetruy, P and Born, M and Bortoluzzi, D and Cavalleri, A and Cesarini, A and Cruise, AM and Danzmann, K and Silva, MDD and Diepholz, I and Dixon, G and Dolesi, R and Fabi, M and Ferraioli, L and Ferroni, V and Finetti, N and Fitzsimons, ED and Freschi, M and Gesa, L and Gibert, F and Giardini, D and Giusteri, R and Grimani, C and Grzymisch, J and Harrison, I and Heinzel, G and Hewitson, M and Hollington, D and Hoyland, D and Hueller, M and Inchauspe, H and Jennrich, O and Jetzer, P and Karnesis, N and Kaune, B and Korsakova, N and Killow, CJ and Laurenza, M and Lobo, JA and Lloro, I and Liu, L and Lopez-Zaragoza, JP and Maarschalkerweerd, R and Mance, D and Martin, V and Martin-Polo, L and Martino, J and Martin-Porqueras, F and Mateos, I and McNamara, PW and Mendes, J and Mendes, L and Nofrarias, M and Paczkowski, S and Perreur-Lloyd, M and Petiteau, A and Pivato, P and Plagnol, E and Ramos-Castro, J and Reiche, J },
doi = {1538-4357/aaa774},
journal = {Astrophysical Journal},
title = {Characteristics and energy dependence of recurrent galactic cosmic-ray Flux depressions and of a Forbush decrease with LISA Pathfinder},
url = {http://dx.doi.org/10.3847/1538-4357/aaa774},
volume = {854},
year = {2018}
}

RIS format (EndNote, RefMan)

TY  - JOUR
AB - 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.
AU - Armano,M
AU - Audley,H
AU - Baird,J
AU - Bassan,M
AU - Benella,S
AU - Binetruy,P
AU - Born,M
AU - Bortoluzzi,D
AU - Cavalleri,A
AU - Cesarini,A
AU - Cruise,AM
AU - Danzmann,K
AU - Silva,MDD
AU - Diepholz,I
AU - Dixon,G
AU - Dolesi,R
AU - Fabi,M
AU - Ferraioli,L
AU - Ferroni,V
AU - Finetti,N
AU - Fitzsimons,ED
AU - Freschi,M
AU - Gesa,L
AU - Gibert,F
AU - Giardini,D
AU - Giusteri,R
AU - Grimani,C
AU - Grzymisch,J
AU - Harrison,I
AU - Heinzel,G
AU - Hewitson,M
AU - Hollington,D
AU - Hoyland,D
AU - Hueller,M
AU - Inchauspe,H
AU - Jennrich,O
AU - Jetzer,P
AU - Karnesis,N
AU - Kaune,B
AU - Korsakova,N
AU - Killow,CJ
AU - Laurenza,M
AU - Lobo,JA
AU - Lloro,I
AU - Liu,L
AU - Lopez-Zaragoza,JP
AU - Maarschalkerweerd,R
AU - Mance,D
AU - Martin,V
AU - Martin-Polo,L
AU - Martino,J
AU - Martin-Porqueras,F
AU - Mateos,I
AU - McNamara,PW
AU - Mendes,J
AU - Mendes,L
AU - Nofrarias,M
AU - Paczkowski,S
AU - Perreur-Lloyd,M
AU - Petiteau,A
AU - Pivato,P
AU - Plagnol,E
AU - Ramos-Castro,J
AU - Reiche,J
AU - Robertson,DI
AU - Rivas,F
AU - Russano,G
AU - Sabbatini,F
AU - Slutsky,J
AU - Sopuerta,CF
AU - Sumner,T
AU - Telloni,D
AU - Texier,D
AU - Thorpe,JI
AU - Vetrugno,D
AU - Vitale,S
AU - Wanner,G
AU - Ward,H
AU - Wass,P
AU - Weber,WJ
AU - Wissel,L
AU - Wittchen,A
AU - Zambotti,A
AU - Zenoni,C
AU - Zweifel,P
DO - 1538-4357/aaa774
PY - 2018///
SN - 0004-637X
TI - Characteristics and energy dependence of recurrent galactic cosmic-ray Flux depressions and of a Forbush decrease with LISA Pathfinder
T2 - Astrophysical Journal
UR - http://dx.doi.org/10.3847/1538-4357/aaa774
UR - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000425389700011&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR - http://hdl.handle.net/10044/1/58056
VL - 854
ER -