@Article{SantosSobAbdSouTak:2004:PlBuZo,
author = "Santos, Pedrina Morais Terra dos and Sobral, Jos{\'e} Humberto
Andrade and Abdu, Mangalathayil Ali and Souza, Jonas Rodrigues de
and Takahashi, Hisao",
affiliation = "{Instituto Nacional de Pesquisas Espaciais. Divis{\~a}o de
Aeronomia (INPE.DAE)} and {Instituto Nacional de Pesquisas
Espaciais. Divis{\~a}o de Aeronomia (INPE.DAE)} and {Instituto
Nacional de Pesquisas Espaciais. Divis{\~a}o de Aeronomia
(INPE.DAE)} and {Instituto Nacional de Pesquisas Espaciais.
Divis{\~a}o de Aeronomia (INPE.DAE)} and {Instituto Nacional de
Pesquisas Espaciais. Divis{\~a}o de Aeronomia (INPE.DAE)}",
title = "Plasma bubble zonal velocity variations with solar activity in the
Brazilian region",
journal = "Annales Geophysicae",
year = "2004",
volume = "22",
number = "9",
pages = "3123--3128",
keywords = "AERONOMY, Ionosphere, Ionospheric irregularities, Instruments and
techniques, Atmospheric composition and structure, Airglow and
aurora, Equatorial ionosphere, Airglow observations, Cachoeira
Paulista, Low-latitude, Drifts, Irregularities, Depletions,
Dynamics, Gradient, AERONOMIA, Ionosfera, Irregularidades
ionosf{\'e}ricas, Composi{\c{c}}{\~a}o e estrutura
atmosf{\'e}rica, Ionosfera equatorial, Din{\^a}mica,
Gradiente.",
abstract = "A statistical study of the zonal drift velocities of the
ionospheric plasma bubbles using experimental airglow data
acquired at the low-latitude station Cachoeira Paulista (Geogr.
22.5degrees S, 45degrees W, dip angle 28degrees S) during the
period of October to March, between 1980 and 1994, is presented
here. This study is based on 109 nights of zonal plasma bubble
velocity estimations as determined from bubbles signatures on the
01630 rim scanning photometer airglow data. The zonal velocity
magnitudes of the plasma bubbles are investigated with respect to
solar activity and local time. It is verified that these
velocities tend to increase with the solar EUV flux, using the
solar 10.7-cm radio flux as a proxy (F10.7). These velocities are
seen to be larger during the solar maximum activity period than in
the solar minimum period. As to the local time variation. they are
seen to peak before midnight, in the 20:30-22:30 LT time frame,
depending on the season. The all-data plot based on the 109 nights
of airglow experiments shows that the plasma bubble mean zonal
drift velocities tend to decrease with local time, but they peak
at 22:25 LT, where the velocity magnitude reaches 127.4 ms(-1).
The zonal drift variations with local time and solar flux are
shown in Figs. 1 and 2, respectively.",
copyholder = "SID/SCD",
issn = "0992-7689",
language = "en",
targetfile = "plasma bubble.pdf",
urlaccessdate = "19 maio 2024"
}