CV Lattes
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Ministério da Ciência, Tecnologia e Inovação (Brasil). Instituto Nacional de Pesquisas Espaciais (INPE) (Institutional affiliation from the last research proposal) Birthplace: Brazil
graduation at Engenharia Elétrica from Universidade Federal de Santa Maria (2008), master's at Geophysics from Instituto Nacional de Pesquisas Espaciais (2011) and doctorate at Geophysics from Instituto Nacional de Pesquisas Espaciais (2015). Has experience in Aerospace Engineering, focusing on Satellites and Other Aerospace Devices, acting on the following subjects: clima espacial and raios cósmicos de alta energia. (Source: Lattes Curriculum)
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This project aims to study coronal mass ejections (CMEs), its resulting structures in the interplanetary medium (ICMEs) and interplanetary shocks in a comprehensive and detailed way. Observations from coronagraphs onboard both the twin spacecraft STEREO (Solar Terrestrial Relations Observatory) and the SOHO (Solar and Heliospheric Observatory) will be used. In the Earth vicinity, the obs…
This project aims to study coronal mass ejections (CMEs) and their interplanetary counterparts (ICMEs) using observations from both ground-based cosmic ray detectors and coronagraphs. It is known that CMEs are one of the main sources of geomagnetic disturbances (Gosling et al. 1990, 1991), being a central role on space weather research. The combination of ground-based cosmic ray (muon) d…
It is the objective of this project to study solar-interplanetary-geomagnetic disturbances, such as solar and interplanetary coronal mass ejections (CMEs and ICMEs), using satellite data and ground-based cosmic ray observations, in order to improve Space Weather forecasting. Large Angle and Spectroscopic Coronagraph (LASCO) and Extreme Ultraviolet Imaging Telescope (EIT), aboard the Solar…
Coronal mass ejections (CMEs) are the main drivers of geomagnetic storms. Hence, prediction of their arrival time at Earth is of primary interest for understanding and improving Space Weather. To do this it is necessary to understand the forces acting during their propagation from the Sun to the Earth, such as the Lorentz hoop force and the aerodynamic drag. Some models, such as the erup…
Cosmic ray with energy on the GeV range are modulated in the vicinity of the Earth by interplanetary structures like magnetic clouds. The interplanetary magnetic structures affect specially the diffusion and convection of cosmic ray. Thanks to the simultaneous observation of secondary cosmic ray (muons) in different places on the Earth surface, it is possible to reconstruct the spatial di…
| 3 / 3 | Completed scholarships in Brazil |
| 2 / 2 | Completed scholarships abroad |
| 5 / 5 | All Scholarships |
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