%0 Journal Article
%4 sid.inpe.br/mtc-m21b/2014/05.30.02.18.57
%2 sid.inpe.br/mtc-m21b/2014/05.30.02.18.58
%@doi 10.1088/1742-6596/484/1/012012
%@issn 1742-6588
%F scopus 2014-05 DaSilvaCostaAgui:2014:MiMaSc
%T Spherical gravitational wave detectors: MiniGRAIL and Mario Schenberg
%D 2014
%9 conference paper
%A Costa, Carlos Filipe da Silva,
%A Aguiar, Odylio Denys de,
%@affiliation Universidade de São Paulo (USP)
%@affiliation Instituto Nacional de Pesquisas Espaciais (INPE)
%@electronicmailaddress filipe.dasilva@usp.br
%@electronicmailaddress odylio.aguiar@inpe.br
%B Journal of Physics: Conference Series
%V 484
%N 1
%K Gravitational effects, Gravity waves, Spheres, Data analysis techniques, Directional detections, Gravitational wave detectors, Independent channels, Low latency, Off-line analysis, Sensitivity improvements, Spherical detectors, Detectors.
%X Spherical gravitational wave detectors allow the analysis of multiple independent channels and, therefore, are able to determine gravitational wave directions and polarizations. There are two spherical detectors being developed now: MiniGRAIL (Netherlands) and Mario Schenberg (Brazil). Both share the same principle of detection and main features. They have done commissioning runs and shown progress in their development. We have presented here the status of Mario Schenberg. Its transducers have been redesigned for sensitivity improvements. While an offline analysis was already developed for MiniGRAIL, we have investigated a low latency data analysis technique for Mario Schenberg. Both analysis are based on directional detection. © Published under licence by IOP Publishing Ltd.
%@language en
%3 1742-6596_484_1_012012.pdf
%O Proceedings of the 7th International Conference on Gravitation and Cosmology (ICGC201