@Article{FagundesAbBiSaFrPiLi:2009:2.TrPl,
author = "Fagundes, Paulo Roberto and Abalde, Jose Ricardo and Bittencourt,
Jos{\'e} Augusto and Sahai, Yogeshwar and Francisco, Rosalia
Gomes and Pillat, Valdir Gil and Lima, Washington Lima C.",
affiliation = "{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and
{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Universidade do Vale do
Para{\'{\i}}ba (UNIVAP)} and {Universidade do Vale do
Para{\'{\i}}ba (UNIVAP)} and {Centro Universit{\'a}rio Luterano
de Palma}",
title = "F layer postsunset height rise due to electric field prereversal
enhancement: 2. Traveling planetary wave ionospheric disturbances
and their role on the generation of equatorial spread F",
journal = "Journal of Geophysical Research",
year = "2009",
volume = "114",
number = "A12322",
month = "Dec.",
keywords = "region plasma depletions, to-day variability, onset conditions,
solar-activity, gravity-wave, bubbles, signatures, NM,
mesosphere.",
abstract = "This paper investigates the role played by traveling planetary
wave ionospheric disturbances (TPWIDs) on the modulation of the
electric field prereversal enhancement (PRE) amplitude,
near-sunset hours, in the equatorial ionosphere, and their
influence on the day-to-day equatorial spread F (ESF) variability.
We show that {"}fresh'' (ESF) day-to-day variability is closely
related with the postsunset height rise due to the electric field
PRE, and there is some indication that the altitude of 300 km may
be a threshold height for the generation of fresh ESF.
Observations of F layer virtual heights during evening hours (1800
LT, 1900 LT, and 2000 LT) present a strong day-to-day variability,
even during geomagnetically quiet periods. In fact, this
well-organized variability is induced by TPWIDs-type oscillations
that push the F layer up or down according to the TPWID phase. The
preliminary analysis presented here show that, when the planetary
TPWID oscillations or geomagnetic activity raises the F layer
around sunset hours, the occurrence of fresh ESF is increased, but
when the TPWID-type oscillations or geomagnetic activity pushes
the F layer downward, the fresh ESF occurrence is reduced. Also,
the TPWID phase modulated the onset time of the fresh ESF during
high fresh ESF season. The modulation acts in such way that, when
the TPWID phase maximizes, the fresh ESF onset time occurs earlier
than when the TPWID phase minimizes and the fresh ESF onset time
occurs later.",
doi = "10.1029/2009JA014482",
url = "http://dx.doi.org/10.1029/2009JA014482",
issn = "0148-0227",
label = "lattes: 1106857072073407 6 FagundesAbBiSaFrPiLi:2009:PAIITR",
language = "en",
urlaccessdate = "04 maio 2024"
}