Mostra el registre d'ítem simple
Interpolation of the magnetic field at the test masses in eLISA
dc.contributor.author | Mateos, I. |
dc.contributor.author | Díaz Aguiló, Marc |
dc.contributor.author | Ramos Castro, Juan José |
dc.contributor.author | García-Berro Montilla, Enrique |
dc.contributor.author | Lobo, J.A. |
dc.contributor.other | Universitat Politècnica de Catalunya. Departament d'Enginyeria Electrònica |
dc.contributor.other | Universitat Politècnica de Catalunya. Departament de Física |
dc.date.accessioned | 2015-11-05T15:20:32Z |
dc.date.available | 2016-11-07T01:30:20Z |
dc.date.issued | 2015-08-20 |
dc.identifier.citation | Mateos, I., Diaz-Aguilo, M., Ramos, J., Garcia-berro, E., Lobo, J.A. Interpolation of the magnetic field at the test masses in eLISA. "Classical and quantum gravity", 20 Agost 2015, vol. 32, núm. 16. |
dc.identifier.issn | 0264-9381 |
dc.identifier.uri | http://hdl.handle.net/2117/78841 |
dc.description.abstract | A feasible design for a magnetic diagnostics subsystem for eLISA will be based on that of its precursor mission, LISA Pathfinder. Previous experience indicates that magnetic field estimation at the positions of the test masses has certain complications. This is due to two reasons. The first is that magnetometers usually back-act due to their measurement principles (i.e., they also create their own magnetic fields), while the second is that the sensors selected for LISA Pathfinder have a large size, which conflicts with space resolution and with the possibility of having a sufficient number of them to properly map the magnetic field around the test masses. However, high-sensitivity and small-sized sensors that significantly mitigate the two aforementioned limitations exist, and have been proposed to overcome these problems. Thus, these sensors will be likely selected for the magnetic diagnostics subsystem of eLISA. Here we perform a quantitative analysis of the new magnetic subsystem, as it is currently conceived, and assess the feasibility of selecting these sensors in the final configuration of the magnetic diagnostic subsystem. |
dc.language.iso | eng |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/es/ |
dc.subject | Àrees temàtiques de la UPC::Física::Relativitat::Gravitació |
dc.subject.lcsh | Gravitational waves |
dc.subject.other | LISA |
dc.subject.other | Gravitational wave detector |
dc.subject.other | LISA Pathfinder |
dc.subject.other | Magnetometer |
dc.subject.other | Magnetic diagnostics |
dc.subject.other | Sensors |
dc.title | Interpolation of the magnetic field at the test masses in eLISA |
dc.type | Article |
dc.subject.lemac | Ones gravitacionals |
dc.contributor.group | Universitat Politècnica de Catalunya. GAA - Grup d'Astronomia i Astrofísica |
dc.identifier.doi | 10.1088/0264-9381/32/16/165003 |
dc.description.peerreviewed | Peer Reviewed |
dc.relation.publisherversion | http://iopscience.iop.org/article/10.1088/0264-9381/32/16/165003/meta;jsessionid=9DE284DEE1FC0956394139D733B3D39F.c1.iopscience.cld.iop.org |
dc.rights.access | Open Access |
local.identifier.drac | 16842853 |
dc.description.version | Postprint (author's final draft) |
dc.relation.projectid | info:eu-repo/grantAgreement/MICINN//AYA2011-23102/ES/ENANAS BLANCAS: PROGENITORES, EVOLUCION, PULSACIONES Y EXPLOSIONES/ |
local.citation.author | Mateos, I.; Diaz-Aguilo, M.; Ramos, J.; Garcia-berro, E.; Lobo, J.A |
local.citation.publicationName | Classical and quantum gravity |
local.citation.volume | 32 |
local.citation.number | 16 |
Fitxers d'aquest items
Aquest ítem apareix a les col·leccions següents
-
Articles de revista [2.209]
-
Articles de revista [299]
-
Articles de revista [1.729]