@Article{Agyei-YeboahPMBPELTW:2019:SeVaPl,
author = "Agyei-Yeboah, Ebenezer and Paulino, Igo and Medeiros, Amauri
Fragaso and Buriti, Ricardo Arlen and Paulino, Ana Roberta and
Essien, Patrick and Lomotey, Solomon Otoo and Takahashi, Hisao and
Wrasse, Cristiano Max",
affiliation = "{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and
{Universidade Federal de Campina Grande (UFCG)} and {Universidade
Federal de Campina Grande (UFCG)} and {Universidade Federal de
Campina Grande (UFCG)} and {Universidade Federal de Campina Grande
(UFCG)} 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 = "Seasonal variation of plasma bubbles during solar cycle 23–24 over
the Brazilian equatorial region",
journal = "Advances in Space Research",
year = "2019",
volume = "64",
number = "7",
pages = "1365--1374",
month = "Oct.",
keywords = "Solar cycle, Plasma bubbles, All-sky imaging, Equatorial
ionosphere.",
abstract = "In this study, OI 630.0 nm nightglow image data obtained from an
all-sky imaging station located at Sao Joao do Cariri (7.4S, 36.5
W), have been used to study the occurrence of equatorial plasma
bubbles (EPBs) over the Brazilian equatorial region. The
observations, which took place from September 2000 to December
2010 (almost eleven years), covered a significant part of solar
cycle 23 (descending phase of SC23) and the very beginning of
solar cycle 24 (ascending phase of SC24). There were 1337 nights
of observations with 666 nights with EPB events, which translates
to an occurrence rate of 49.8%. Of these nights, 1290 were
considered quiet (Dst - 50 nT) with 50% plasma bubbles occurrence
rate. The occurrence of EPBs was studied under three solar
activity phases high solar activity phase (HSA, September 2000
March 2004), moderate solar activity phase (MSA or descending
phase, March 2004 October 2006) and low solar activity phase (LSA,
October 2006 December 2010). The low solar activity phase is part
of the peculiar solar cycle 24, considered the weakest in over a
century with most sunspotless days (20082009). The maximum
occurrence of bubbles, equal to 54.2%, was found during the HSA
phase, with percentages characterizing MSA and LSA being
respectively 52.4% and 45.8%. The analysis also showed clear
seasonal variation in the EPB occurrence with maximum rates in
summer, spring, autumn, and the minimum rates in winter for all
solar activity phases. Overall, there was observed solar cycle
variation in each season with maximum occurrence in HSA followed
by MSA and then LSA except in autumn where higher occurrence rate
was observed in LSA phase than in MSA phase.",
doi = "10.1016/j.asr.2019.06.041",
url = "http://dx.doi.org/10.1016/j.asr.2019.06.041",
issn = "0273-1177 and 1879-1948",
language = "en",
targetfile = "agyei_sesonal.pdf",
urlaccessdate = "15 jun. 2024"
}