Heliospheric influences on LISA

C. Grimani; M. Fabi; N. Finetti; D. Tombolato; L. Marconi; R. Stanga; A. Lobo; M. Chmeissani; C. Puigdengoles

doi:10.1088/0264-9381/26/9/094018

Heliospheric influences on LISA

C. Grimani
, M. Fabi
, N. Finetti
, D. Tombolato
, L. Marconi
, R. Stanga
, A. Lobo
, M. Chmeissani
, C. Puigdengoles

University of Urbino Carlo Bo
Istituto Nazionale di Fisica Nucleare, Sezione di Firenze
Università Dell'Aquila
Laboratori Nazionali del Gran Sasso
Trento Institute for Fundamental Physics and Applications
University of Florence
Institut d’Estudis Espacials de Catalunya (IEEC)
The Barcelona Institute of Science and Technology

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

10 Citations (Scopus)

Résumé

Laser interferometer space antenna (LISA) is the first interferometer devoted to the detection of low frequency gravitational waves in space. Control of the environment and the study of the effects of energetic particles traversing the LISA apparatus are mandatory for this experiment to be fully successful. Telescopes for solar and cosmic-ray particle monitoring will be placed on board LISA and its precursor mission LISA Pathfinder (LISA-PF). In particular, proton, helium and electron detection is recommended on LISA. In this paper, we report expected incident galactic proton and helium fluxes at the time of LISA and LISA-PF missions. The number of solar events with the fluence ranging between 10⁶ and 10¹¹ protons cm^-2 above 30 MeV occurring during the LISA missions is estimated as well. Finally, we discuss the importance of electron detection on LISA to forecast upcoming solar energetic protons.

langue originale	Anglais
Numéro d'article	094018
journal	Classical and Quantum Gravity
Volume	26
Numéro de publication	9
Les DOIs	https://doi.org/10.1088/0264-9381/26/9/094018
état	Publié - 7 mai 2009
Modification externe	Oui

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10.1088/0264-9381/26/9/094018

Contient cette citation

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title = "Heliospheric influences on LISA",

abstract = "Laser interferometer space antenna (LISA) is the first interferometer devoted to the detection of low frequency gravitational waves in space. Control of the environment and the study of the effects of energetic particles traversing the LISA apparatus are mandatory for this experiment to be fully successful. Telescopes for solar and cosmic-ray particle monitoring will be placed on board LISA and its precursor mission LISA Pathfinder (LISA-PF). In particular, proton, helium and electron detection is recommended on LISA. In this paper, we report expected incident galactic proton and helium fluxes at the time of LISA and LISA-PF missions. The number of solar events with the fluence ranging between 106 and 1011 protons cm-2 above 30 MeV occurring during the LISA missions is estimated as well. Finally, we discuss the importance of electron detection on LISA to forecast upcoming solar energetic protons.",

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T1 - Heliospheric influences on LISA

AU - Grimani, C.

AU - Fabi, M.

AU - Finetti, N.

AU - Tombolato, D.

AU - Marconi, L.

AU - Stanga, R.

AU - Lobo, A.

AU - Chmeissani, M.

AU - Puigdengoles, C.

PY - 2009/5/7

Y1 - 2009/5/7

N2 - Laser interferometer space antenna (LISA) is the first interferometer devoted to the detection of low frequency gravitational waves in space. Control of the environment and the study of the effects of energetic particles traversing the LISA apparatus are mandatory for this experiment to be fully successful. Telescopes for solar and cosmic-ray particle monitoring will be placed on board LISA and its precursor mission LISA Pathfinder (LISA-PF). In particular, proton, helium and electron detection is recommended on LISA. In this paper, we report expected incident galactic proton and helium fluxes at the time of LISA and LISA-PF missions. The number of solar events with the fluence ranging between 106 and 1011 protons cm-2 above 30 MeV occurring during the LISA missions is estimated as well. Finally, we discuss the importance of electron detection on LISA to forecast upcoming solar energetic protons.

AB - Laser interferometer space antenna (LISA) is the first interferometer devoted to the detection of low frequency gravitational waves in space. Control of the environment and the study of the effects of energetic particles traversing the LISA apparatus are mandatory for this experiment to be fully successful. Telescopes for solar and cosmic-ray particle monitoring will be placed on board LISA and its precursor mission LISA Pathfinder (LISA-PF). In particular, proton, helium and electron detection is recommended on LISA. In this paper, we report expected incident galactic proton and helium fluxes at the time of LISA and LISA-PF missions. The number of solar events with the fluence ranging between 106 and 1011 protons cm-2 above 30 MeV occurring during the LISA missions is estimated as well. Finally, we discuss the importance of electron detection on LISA to forecast upcoming solar energetic protons.

U2 - 10.1088/0264-9381/26/9/094018

DO - 10.1088/0264-9381/26/9/094018

M3 - Article

AN - SCOPUS:77955129023

SN - 0264-9381

VL - 26

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 9

M1 - 094018

ER -

Heliospheric influences on LISA

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