@InProceedings{ResendeDBBMPCBCBS:2018:ClStQu,
author = "Resende, Laysa Cristina Ara{\'u}jo and Denardin, Clezio Marcos
and Batista, Inez Staciarini and Bertollotto, Thaina de Oliveira
and Moro, Juliano and Pican{\c{c}}o, Giorgio Arlan da Silva and
Chen, Sony Su and Biliblio, Anderson Vestena and Carmo, Carolina
de Sousa do and Barbosa Neto, Paulo Fran{\c{c}}a and Silva, R.
P.",
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
{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 = "Climatological study and qualification of a new ionospheric plasma
index to study the irregularities in the F region",
year = "2018",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 7. (SBGEA)",
abstract = "Vertical drifts of the F region at the dip equator are
characterized by the interaction of the ionospheric plasma with
the zonal electric field and the Earth's magnetic field. Abrupt
variations on the drift are strongly associated with the
occurrence of plasma irregularities during the nighttime periods,
which are manifestations of the space weather on the ionosphere
environment involving the solar-terrestrial interaction without
necessarily, require magnetic storms. In this context, the
Brazilian Space Weather Study and Monitoring Program (Embrace) of
the National Institute for Space Research (INPE) has been
developing different indexes that describe these ionospheric
effects in the Brazilian sector. Therefore, the main purpose of
this work was to produce a new ionospheric scale based on the
analysis of the ionospheric plasma drift velocity. Thus, it was
developed a careful analysis using the virtual height parameter,
hF. This ionospheric parameter is provided by a high frequency
radar, or Digisonde, for the near equatorial region, S{\~a}o
Lu{\'{\i}}s (2°S, 44° O, I: -2.3°). In this study we analyzed 10
years of data divided in season, magnetic activity and phase of
the solar cycle in order to construct a standardized scale. The
results of this new index allow us evaluating the impacts of
ionospheric phenomena in the Space Weather environment recently.",
conference-location = "Santa Maria, RS",
conference-year = "05-09 nov",
language = "pt",
urlaccessdate = "10 maio 2024"
}