@InProceedings{NeelakshiRoOdKhMeMuSt:2018:MuAnEq,
author = "Neelakshi, Joshi and Rosa, Reinaldo Roberto and Odriozola, Siomel
Savio and Kherani, Esfhan Alam and Meneses J{\'u}nior, Francisco
Carlos de and Muralikrishna, Polinaya and Stephany, Stephen",
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)}",
title = "Multifractal analysis of equatorial E-F transition region in-sity
data",
year = "2018",
organization = "Simp{\'o}sio Brasileiro de Geof{\'{\i}}sica Espacial e
Aeronomia, 7. (SBGEA)",
abstract = "In this study, we present multifractal analysis of the equatorial
E-F transition region data obtained from an in-situ experiment
performed at Alc{\^a}ntara (2.4°S; 44.4°W), Brazil. Earlier
investigations (Odriozola et al., 2017) on this data indicated the
presence of smallmedium scale irregularities in the valley region.
At the time of launch, ground based equipment detected conditions
favorable for the generation of plasma bubbles in F-region. Also,
this experiment can be considered as the first to detect a
scenario similar to the one observed in the RTI maps at Jicamara
(Woodman and Chau, 2001). Multifractal Detrended Fluctuation
Analysis (MFDFA) and P-model (Meneveau and Sreenivasan, 1987) fit
is used to analyze the electron density time series. Analysis of
the scaling pattern obtained from the singularity spectra and
fitted p-values help to understand the nature of ionospheric
turbulence in E-F transition region. The multifractal structure
function is able to characterize nonlinear spatio-temporal
behavior and complex processes such as non-homogenous energy
cascades that could be present in the Ionospheric plasma bubble
region. This procedure is relatively unprecedented since studies
of equatorial E-region and the intermediate region between the E
and F layers at nighttime are scarce. Power spectral density (PSD)
obtained from this data has shown the presence of dual slope under
small-medium scale irregularities. Preliminary results show the
PSD slope varies as 0. 9<\β1< . for medium and 0. 4<
\β2<3. for small scales and energy cascading probability as
0.15 < p < 0.4 suggesting that the main underlying physical
process is a nonhomogeneous multiplicative cascade.",
conference-location = "Santa Maria, RS",
conference-year = "05-09 nov",
language = "pt",
urlaccessdate = "28 abr. 2024"
}