Physics
Scientist
Instituto Nacional de Pesquisas Espaciais, São José dos Campos, São Paulo, Brazil
National Institute for Space Research, São José dos Campos, Brazil
Divisão de Geofísica Espacial, Instituto Nacional de Pesquisas Espaciais, Av. dos Astronautas 1758, Jardim da Granja 12227010, P.O. Box 515, São José dos Campos, São Paulo, Brazil
Instituto Nacional de Pesquisas Espaciais-INPE / MCT, Ave. dos Astronautas, 1758, PO Box 515, Sao Jose dos Campos, SP 12227-010 Brazil
Divisão de Geofísica Espacial, Instituto Nacional de Pesquisas Espaciais, Av. dos Astronautas, 1758, Jardim da Granja, 12227010, P.O. Box 515, São José dos Campos, São Paulo, Brazil
Instituto Nacional Pesquisas Espaciais, INPE, CP 515, So José dos Campos, 12201-970-, So Paulo, Brazil
Instituto Nacional de Pesquisas Espaciais, INPE, CP 515, São José dos Campos, 12201-970, SP, Brazil
Instituto Nacional de Pesquisas Espaciais, INPE, CP 515, São José dos Campos, 12201-970, SP, Brazil, BR
Instituto Nacional de Pesquisas Espaciais, Sao Jose dos Campos, Brazil
INPE, Space Geophysic Division, Sao Jose dos Campos, SP, Brazil
INPE, CP 515, Sao Jose dos Campos, SP 12201-970 Brazil
Instituto Nacional de Pesquisas Espaciais, CP 515, Sao Jose dos Campos, SP 12201-970 Brazil
Instituto Nacional Pesquisas Espaciais, CP 515, Sáo José dos Campos, Sáo Paulo 12201-970, Brazil
Geofísica Espacial, Instituto Nacional de Pesquisas Espaciais, Sao Jose dos Campos, Brazil
National Institute for Space Research-INPE / MCT, CP 515, 12245-970 São José dos Campos, SP, Brazil
National Institute of Space Research
Instituto Nacional de Pesquisas Espaciais, Av. dos Astronautas, 1758, Jardim da Granja, 12227010, São José dos Campos, São Paulo, Brazil Nacional de Pesquisas Espacias
3D Coronal Observations and Sun Earth Connections : from SOHO to STEREO data
A Study of Geoeffective Magnetic Clouds in the Interplanetary Medium
A study of magnetic storms development in two or more steps and its association with the polarity of magnetic clouds
A Tool For Improved Space Weather Predictions: The CME Expansion Speed
An Akasofu's Epsilon Parameter Corrected By The Solar Wind Dynamic Pressure As A Guide For The Energy Balance Estimate During Geomagnetic Storms
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