@InProceedings{RodríguezGómesVieiDalLPala:2018:CoElDe,
author = "Rodr{\'{\i}}guez G{\'o}mes, Jenny Marcela and Vieira,
Lu{\'{\i}}s Eduardo Antunes and Dal Lago, Alisson and Palacios,
J.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Universidad de Alcal{\'a}}",
title = "Coronal electron density temperature and solar spectral irradiance
during solar cycles 23 and 24",
year = "2018",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 7. (SBGEA)",
abstract = "Plasma parameters such as the electron density and temperature
play a key role in the dynamics of the solar atmosphere. These
characteristics are important in solar physics because they can
help us to understand the physics of the solar corona, the
ultimate goal being the reconstruction of the electron density and
temperature distributions in the solar corona. We present a
physics-based model to reconstruct the density, temperature, and
emission in the EUV band. This model, called COronal DEnsity and
Temperature (CODET), is composed of a flux transport model, an
extrapolation model, an emission model, and an optimization
algorithm. The CODET model parameters were constrained by
comparing the models output to the TIMED/SEE record instead of
direct observations because it covers a longer time interval than
the direct solar observations currently available. The most
important results of the current work are the recovery of SSI
variability in specific wavelengths in the EUV band, as well as
the variations in density and temperature during the solar cycle
23 and 24, through the solar atmosphere with the CODET model.",
conference-location = "Santa Maria, RS",
conference-year = "05-09 nov",
language = "pt",
targetfile = "rodriguez_coronal.pdf",
urlaccessdate = "19 abr. 2024"
}