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Analysis and interpretation of high energy processes in solar flares

Grant number: 09/15880-0
Support type:Research Grants - Visiting Researcher Grant - International
Duration: October 15, 2010 - April 14, 2011
Field of knowledge:Physical Sciences and Mathematics - Astronomy
Principal Investigator:Pierre Kaufmann
Grantee:Pierre Kaufmann
Visiting researcher: Gerard Trottet
Visiting researcher institution: Observatoire de Paris, France
Home Institution: Escola de Engenharia (EE). Universidade Presbiteriana Mackenzie (UPM). Instituto Presbiteriano Mackenzie. São Paulo, SP, Brazil
Associated research grant:06/06847-1 - Solar activity emissions from submillimeter waves to infrared (SIRA), AP.TEM

Abstract

The program proposes the development of researches concentrated on unique results obtained by the Brazilian Solar Submillimeter Telescope (SST) and recent 10 micron solar observations, operated at El Leoncito, Argentina. Emphasis will be given to the study of emission processes that produce double spectral components at microwaves and in the THz range in combination with measurements in other spectral domains (gamma-rays, X-rays, EUV, optical) in order to further investigate this question by: (i) studying the relationship between sub-millimeter and high energy (> 10 MeV) gamma-rays; (ii) comparing the time evolution of the sub-millimeter emission with that of the associated chromospheric and photospheric responses seen in other spectral domains (chromospheric and photospheric lines, white light, near and mid-infrared). The research should contribute for better understanding of solar flare mechanisms producing high-energy electrons, high-energy positrons, proton beams, and emission processes as a combination of coherent and incoherent processes. (AU)

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)
TROTTET, G.; RAULIN, J.-P.; DE CASTRO, G. GIMENEZ; LUETHI, T.; CASPI, A.; MANDRINI, C. H.; LUONI, M. L.; KAUFMANN, P. Origin of the Submillimeter Radio Emission During the Time-Extended Phase of a Solar Flare. SOLAR PHYSICS, v. 273, n. 2, p. 339-361, NOV 2011. Web of Science Citations: 18.

Please report errors in scientific publications list by writing to: cdi@fapesp.br.