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Analysis of the time evolution of radio emission of solar flares in inhomogeneous environment

Grant number: 08/09339-2
Support Opportunities:Scholarships in Brazil - Post-Doctoral
Effective date (Start): May 01, 2009
Effective date (End): April 30, 2011
Field of knowledge:Physical Sciences and Mathematics - Astronomy - Solar System Astronomy
Principal Investigator:Carlos Guillermo Giménez de Castro
Grantee:Paulo José de Aguiar Simões
Host Institution: Escola de Engenharia (EE). Universidade Presbiteriana Mackenzie (UPM). Instituto Presbiteriano Mackenzie. São Paulo , SP, Brazil


This post-doctoral project aims to analyze solar flares and its inhomogeneous environment. Solar events observed at frequencies that range from 1 to 405 GHz will be investigated by applying techniques that the candidate has been developing in the past few years. These techniques allow a tridimensional description of the magnetic environment where the solar flare occurs, plus the evaluation of the dynamic and distribution evolution of the accelerated electrons and the radio emission that they produce, including full radioactive transfer through the source. Homogeneous models will become obsolete by the new instruments and techniques of solar flare observation, thus this project will help us to understand the present and new observational data and will raise new questions for further investigations. (AU)

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Scientific publications
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
OSBORNE, CHRISTOPHER M. J.; SIMOES, PAULO J. A.. Thyr: a volumetric ray-marching tool for simulating microwave emission. Monthly Notices of the Royal Astronomical Society, v. 485, n. 3, p. 3386-3397, . (08/09339-2, 09/18386-7, 03/03406-6, 04/14248-5)

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