@InProceedings{CuevaPaulKher:2013:StAnMo,
author = "Cueva, Ricardo Yvan de La Cruz and Paula, Eurico Rodrigues de and
Kherani, Esfhan Alam",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Statistical analysis and modelling of equatorial spread F
parameters obtained from VHF radar at three longitudinal sectors",
booktitle = "Proceedings...",
year = "2013",
organization = "International Congress of the Brazilian Geophysical Society and
EXPOGEf, 13.",
note = "Setores de Atividade: Outras atividades profissionais,
cient{\'{\i}}ficas e t{\'e}cnicas.",
keywords = "modelling of spread F parameters, VHF radar plume.",
abstract = "Equatorial Spread F (ESF) is a manifestation of ionospheric
interchange instabilities in the nighttime equatorial F region.
These instabilities generate plasma density irregularities with
scale sizes ranging from kilometers to thousands of kilometers. In
the present study, statistics of various aspects of spread F
occurrence are presented from HF/VHF radar located at three
equatorial stations: Christmas Island (2o N, 202.6o E, 2.9o N dip
latitude, VHF radar), S{\~a}o Lu{\'{\i}}s (2.59o S, 315.8o E,
0.5o S dip latitude, HF radar) and Jicamarca (12o S, 283.1o E,
0.6o N dip latitude). The spread F parameters presented here are
the onset altitude and onset time (onset refers to first
appearance of signal in the radar field of view) of the
bottom-type and plume, and the peak altitude of the plume which
are known to be associated with the spread F occurrence
characteristics. The study reveals novel features namely, seasonal
and solar flux dependence of spread F occurrence over Christmas
island /S{\~a}o Lu{\'{\i}}s, and longitudinal dependence of
spread F occurrence characteristics from these three stations
based on the chosen parameters. The importance of this work lies
in the spread F parameter empirical model developed combining
statistical analysis of three equatorial and longitudinally
separated stations, which is important to study evolution of
irregularities in different longitudinal sectors for space weather
forecasting and nowcasting programs, and improving scintillation
warning models. These parameters show generally linear correlation
with solar flux index (F10.7 cm) and variation with season and
magnetic declination angle. The fit correlation with F10.7cm is
shown as useful information to implement one spread-F development
empirical model based on small scale irregularities detected by
VHF radars.",
conference-location = "Rio de Janeiro",
conference-year = "2013",
label = "lattes: 5569424161133651 1 CuevaPaulKher:2013:StAnMo",
language = "en",
url = "http://sys2.sbgf.org.br/congresso/abstracts/trabalhos/sbgf_4231.pdf",
urlaccessdate = "04 maio 2024"
}