@Article{SobralBABSZTN:1997:PoWi63,
author = "Sobral, Jos{\'e} Humberto Andrade and Borba, Gilvan L. and Abdu,
Mangalathayil Ali and Batista, Inez Staciarini and Sawant,
Hanumant Shankar and Zamlutti, Carlos Jos{\'e} and Takahashi,
Hisao and Nakamura, Y",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Universidade Federal do Rio Grande do Norte-UFRN} 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)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Post-sunset wintertime 630.0 nm airglow perturbations associated
with gravity waves at low latitudes in the South America sector",
journal = "Journal of Atmospheric and Solar-Terrestrial Physics",
year = "1997",
volume = "59",
number = "13",
pages = "1611--1623",
keywords = "aeronomia, atl{\^a}ntico sul, regi{\~a}o f, oxig{\^e}nio,
ionosfera, ondas de radio, ionossonda, aeronomy, south atlantic, f
region, oxygen, ionosphere, radio waves.",
abstract = "We report photometric southern hemisphere wintertime perturbations
of the nocturnal F-region atomic oxygen 630 nm red line intensity
which are observed to occur concurrently with apparent ionogram
signatures of F-region gravity waves. Such airglow events were
detected on a total of 40 days of experiments. The airglow
experiments were run at Cachoeira Paulista (CP, geographic 22°41'
S, 45°00' W, dip 28°S). The events are characterized by
south-to-north travelling airglow valleys, or depletion events
(SNE). They were obtained from a set of 299 experiments performed
during the period of 10 August 1977 to 4 July 1984. Their
equatorwards velocities, wavelengths and periods vary within the
ranges of 150-300ms^-1, 100-200 km and 15 min - 3 h, respectively.
They appear during the post-sunset period and remain within the
field of view of the meridional scanning photometer from about ten
minutes to a few hours. The SNE were seen to occur more frequently
in July and were absent from September to March. The photometer
scanned +- 75° around zenith in the magnetic meridional and zonal
planes. ionogram. spread-F and VHF polarimeter data that showed no
phase or amplitude scintillations during the SNE indicated no
concurrent existence of equatorial plasma depletions. It is shown
that the SNE are not necessarily related to geomagnetic disturbed
conditions. The present results are, to the authors' knowledge,
the first showing gravity wave effects, near the sunset side of
the solar terminator, on the low-latitude F-region atomic oxygen
red nightglow under undisturbed geomagnetic conditions. The
characteristics of these waves point to the solar terminator as
their source of generation. A series of physical and morphological
features of the phenomena are presented.",
issn = "1364-6826",
label = "8728",
language = "en",
targetfile = "1-s2.0-S1364682696001605-main.pdf",
urlaccessdate = "07 maio 2024"
}