@InProceedings{DenardinCRMBFGCBPSHABNPB:2018:FiScRe,
author = "Denardin, Clezio Marcos and Chen, Sony Su and Resende, Laysa
Cristina Ara{\'u}jo and Moro, Juliano and Bilibio, Andreos
Vestena and Fagundes, Paulo Roberto and Gende, Maur{\'{\i}}cio
Alfredo and Cabrera, Miguel Angel and Bolzan, Maur{\'{\i}}cio
Jos{\'e} Alves and Padilha, Ant{\^o}nio Lopes and Schuch, Nelson
Jorge and Hormaechea, Jos{\'e} L. and Alves, Livia Ribeiro and
Barbosa Neto, Paulo Fran{\c{c}}a and Nogueira, Paulo Alexandre
Bronzato and Pican{\c{c}}o, Giorgio Arlan da Silva and
Bertollotto, Thaina",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "The embrace magnetometer network for south america: first
scientific results",
year = "2018",
organization = "Cospar Scientific Assembly, 42.",
abstract = "The present work is the second of a two-part paper on the Embrace
Magnetometer Network. In this part, we provide some of the first
scientific findings that we have already achieved with this
network. We identified the diurnal and the seasonal natural
variations of the H component. We provided the precise
determination of SSC and SI. We showed that the H amplitudes
derived from the Embrace MagNet during intense magnetic storm are
in very good agreement with the Dst index. We showed that it is
possible to investigate of the effects of the Sq systems response
to the X-class solar flares occurring during daytime under
magnetically quiet conditions.",
conference-location = "Pasadena, California",
conference-year = "14-22 July",
language = "en",
urlaccessdate = "29 mar. 2024"
}