@InProceedings{BarbosaVDASGASRGMVSRP:2018:DeSpSt,
author = "Barbosa, Adriany Rodrigues and Vieira, Lu{\'{\i}}s Eduardo
Antunes and Dal Lago, Alisson and Albuquerque, Braulio Fonseca
Carneiro de and Silva, M. R. and Guarnieri, F. L. and Arruda, M.
V. and Stekel, T. R. C. and Rodriguez Gomes, Jenny Marcela and
Guimar{\~a}es, Wellington Rodrigues and Mendes J{\'u}nior, Odim
and Veiga, T. P. and Silva, M. A. and Rodrigues, V. T. and Paula,
B. L.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Laborat{\'o}rio Nacional de Astrof{\'{\i}}sica (LNA)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)}",
title = "Development of a spectropolarimeter to study the sun's magnetic
field",
year = "2018",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 7. (SBGEA)",
abstract = "The development and optimization of technologies has proved of
extreme value for studies of the solar magnetic field through
solar observations in Earth. An example is the increase quality of
the images obtained by telescopes due to the improvement of the
spatial resolution. Cooperatively with the development of
technologies, the use of techniques such as spectropolarimetry
makes it possible to characterize fine structures and obtain
characteristics of the solar magnetic field. However even with all
the progress, there is still no complete understanding of the
physical processes that lead to the solar activity cyclic
variability and its long-term changes, making detailed studies of
the solar magnetic field more fascinating. A spectropolarimeter
was developed containing sCMOS Cameras, 500mm Aperture Commercial
Telescope, Polarization Kit, Fary-Perot Etalon interferometer,
narrow band filters and all customized optics. In the present
work, we show the preliminary results of observation cycles being
performed, with images captured for more than one hundred
wavelengths (positions in the interferometer) and in 8 states of
polarization. The instrument allows to make observations at
different wavelengths (within an emission band) and with different
polarizations, in order to obtain the estimates of the
distribution of the magnetic field vector in the solar disk
images, providing important data to better understanding the Suns
influence on the Geospace and on Earths Climate.",
conference-location = "Santa Maria, RS",
conference-year = "05-09 nov",
language = "pt",
urlaccessdate = "27 abr. 2024"
}