@Article{JesusSaGuFaAbPiLi:2011:FrIoPa,
author = "Jesus, Rodolfo de and Sahai, Y. and Guarnieri, F. L. and Fagundes,
P. R. and Abreu, Alessandro Jos{\'e} de and Pillat, Valdir Gil
and Lima, W. L. C.",
affiliation = "Univ Vale Paraiba UNIVAP, IP\&D and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and Univ Vale Paraiba UNIVAP, IP\&D
and Univ Vale Paraiba UNIVAP, IP\&D and Univ Vale Paraiba UNIVAP,
IP\&D and {} and Univ Luterana Brasil ULBRA, Ctr Univ Luterano
Palmas CEULP, Palmas, TO",
title = "F-region ionospheric parameters observed in the equatorial and low
latitude regions during medium solar activity in the Brazilian
sector and comparison with the IRI-2007 model results",
journal = "Advances in Space Research",
year = "2011",
volume = "47",
number = "4",
pages = "718--728",
month = "Feb",
keywords = "Ionosphere, F-region, International Reference Ionosphere-2007.",
abstract = "The ionospheric sounding observations using the Canadian Advanced
Digital Ionosondes (CADIs) operational at Palmas (PAL; 10.2
degrees S, 48.2 degrees W; dip latitude 6.6 degrees S; a
near-equatorial station), and Sao Jose dos Campos (SJC, 23.2
degrees S, 45.9 degrees W; dip latitude 17.6 degrees S; a
low-latitude station located under the southern crest of the
equatorial ionospheric anomaly), Brazil, are analyzed during the
different seasons viz., winter (June and July 2003), spring
(September and October 2003), summer (December 2003 and January
2004), and fall (March and April 2004). The period used has medium
solar activity (sunspot number between 77.4 and 39.3). The
seasonal mean variations (using only geomagnetically quiet days)
of the ionospheric parameters foF2 (critical frequency of the
F-region), hpF2 (virtual height at 0.834 foF2; considered to be
close to hmF2 (peak height of the F-region)), and h'F (minimum
virtual height of the F-region) are calculated and compared
between PAL and SJC. The prominent differences between PAL and SJC
are as follows: h'F variations show strong post-sunset enhancement
at PAL during the seasons of spring, summer, and fall; hpF2
variations show pre-sunrise uplifting of the F-layer at both
stations during all the seasons and the hpF2 values during the
daytime are lower at SJC compared with PAL during all the seasons;
the foF2 variations show mid-day bite-out at PAL during all the
seasons and SJC shows strong equatorial ionospheric anomaly during
summer and fall seasons. Also, the seasonal variations of the
ionospheric parameters foF2 and hpF2 (with +/- 1 standard
deviation) observed at PAL and SJC are compared with the IRI-2007
model results of foF2 and hmF2. In addition, variations of the
foF2 and hpF2 observed at SJC are compared with the IRI-2001 model
results of foF2 and hmF2. It should be pointed out that the
ionospheric parameter hpF2 is much easier to obtain using computer
program developed at UNIVAP compared with hmF2 (using POLAN
program). During the daytime due to underlying ionization hpF2
estimated is higher (approximately 50 km) than the true peak
height hmF2. During the nighttime hpF2 is fairly close to hmF2.
The comparison between the foF2 variations observed at PAL and SJC
with the IRI-2007 model results shows a fairly good agreement
during all the seasons. However, the comparison between the hpF2
variations observed at PAL and SJC with the hmF2 variations with
the IRI-2007 model results shows: (1) a fairly good agreement
during the nighttime in all the seasons; (2) the model results do
not show the pre-sunrise uplifting of the F-layer at PAL and SJC
in any season; (3) the model results do not show the post-sunset
uplifting of the F-layer at PAL; (4) considering that, in general,
hpF2 is higher than hmF2 during the daytime by about 50 km, the
model results are in good agreement at PAL and SJC during all the
seasons except summer at SJC, when large discrepancies in the
observed hpF2 and modeled hmF2 are observed. Also, it has been
observed that, in general, hmF2 values for SJC calculated using
IRI-2001 are higher than IRI-2007 during the daytime in winter,
summer, and fall. However, hmF2 values for SJC calculated using
IRI-2001, are lower than IRI-2007 during the nighttime in spring.
(C) 2010 COSPAR. Published by Elsevier Ltd. All rights reserved.",
doi = "10.1016/j.asr.2010.10.020",
url = "http://dx.doi.org/10.1016/j.asr.2010.10.020",
issn = "0273-1177",
label = "lattes: 1106857072073407 6 JesusSaGuFaAbPiLi:2011:FrIoPa",
language = "en",
targetfile = "Jesus-AdvSpaceRes-v-47-n4-p718-28science[2].pdf",
urlaccessdate = "15 jun. 2024"
}