CV Lattes
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Universidade de São Paulo (USP). Instituto de Astronomia, Geofísica e Ciências Atmosféricas (IAG) (Institutional affiliation from the last research proposal) Birthplace: Colômbia
He has a degree in Mathematics and Physics from the university Surcolombiana, Neiva-Colombia (2003), a Master's degree in Fundamental Physics from the university Los Andes, Mérida-Venezuela (2010) and a PhD in Astrophysics from the Instituto Nacional de Pesquisas Espaciais (INPE) São José dos Campos-Brazil (2017). He works mainly in the areas of astronomy, solar physics and plasma dynamics, with lines of research centred on magnetohydrodynamic (MHD) waves, thermal equilibrium in the solar atmosphere and astrophysical plasma heating by wave damping. He has experience in processing images and spectra provided by the TRACE, SDO, GOES and IRIS space probes, with data analysis using Fourier and Wavelet transforms. He also has knowledge of the programming languages IDL, FORTRAN 77, Mathematica and Python. (Source: Lattes Curriculum)
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The plasma of the solar atmosphere loses energy by radiation and need a mechanical source of heat for maintaining the temperature in equilibrium. Many studies show that magneto-acoustic waves can balance the energy in some regions of the solar atmosphere. Specifically, these waves allow us to study the gas dynamic in structures as coronal loops and also to get the values of temperature, d…
Solar atmosphere plasma loses energy through radiation and thermal conduction and thus needs a mechanical heat source to maintain its temperature in equilibrium. In the literature, many theoretical and observational studies show us that magnetohydrodynamic waves can balance the energy in certain regions of the solar atmosphere. These waves allow us to study the gas dynamic in structures s…
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