@InProceedings{SchuchDEDGBMSBHDPRSOMKFKBEDHASSJ:2013:BrCoSp,
author = "Schuch, N. J. and Dal Lago, Alisson and Echer, Ezequiel and
Denardini, Clezio Marcos and Gonzalez, Walter Demetrio and Braga,
Carlos Roberto and Mendon{\c{c}}a, Rafael Rodrigues Souza de and
Souza, Mauricio Rosa de and Bremm, Tiago and Hammerschmitt, Bruno
Knevitz and Deggeroni, Vinicius and Petry, Adriano and Rigozo,
Nivaor R. and Silva, Marlos Rockenbach da and Oliveira, Alexandro
Gerson and Munakata, K and Kato, C. and Fujii, Z and Kuwabara, T
and Bieber, J. W. and Evenson, Paul and Duldig, M. L. and Humble,
J. E. and Al Jassar, H. K. and Sharma, M. M. and Sabbah, I and
Jansen, F.",
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 {} and {} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "The Global Muon Detector Network - GMDN. The Brazilian
Contribution for SpaceWeather Forecasting",
booktitle = "Proceedings...",
year = "2013",
organization = "International Cosmic Ray Conference, 33. (ICRC).",
keywords = "Galactic cosmic rays, muon, coronal mass ejection, space
weather.",
abstract = "The GMDN, is a Global Muon Detector Network (GMDN) of ground based
multi-directional detectors, and an international collaboration
consisting of 10 institutions from 6 countries, with real time
data generated by the GMDN, which was developed at Shinshu
University, Japan. The Brazilian GMDNs contribution was the
installation in 2001, of a Multi-Directional Muon Detector
prototype (MMD) for detection of high-energy galactic cosmic rays
(GCRs), through an international cooperation between Brazil, Japan
and USA, and has been in operation since then at the Southern
Space Observatory - SSO/CRS/INPE - MCTI, (Latitude 29o , 26, 24S,
Longitude 53o , 48, 38W, 492m above sea level), Sao Martinho da
Serra, RS, in southern Brazil. The SSO-MMD detectors capability
and sensitivity were twice upgraded, in 2005 and 2012. The
Brazilian contribution for Space Weather forecasting is through
the observations conducted by the SSO-MMD which are used for
forecasting the arrival of the geomagnetic storm and their
Interplanetary Coronal Mass Ejection (ICME) drivers in the
near-Earth geospace. The detector measures GCRs by detecting
secondary muons produced from the hadronic interactions of primary
GCRs (mostly protons) with atmospheric nuclei. Since muons have a
relatively short life-time (about 2.2 microseconds at rest), it
can reach the ground level due to the relativistic effect, and can
preserving the incident direction of primary particles, because
its high energy, the SSO-MMD detector can measure the GCRs
intensity in 17 directions as a multidirectional detector at a
single location, the SSO in southern Brazil.",
conference-location = "Rio de Janeiro",
conference-year = "2013",
label = "lattes: 4050318480364899 6
SchuchDEDGBMSBHDPRSOMKFKBEDHASSJ:2013:BrCoSp",
language = "en",
targetfile = "ICRC2013-946The Global Muon Detector Network - GMDN. The Brazilian
Contribution for SpaceWeather Forecasting.pdf",
urlaccessdate = "06 maio 2024"
}