@Article{Kane:2009:EvDsAu,
author = "Kane, Rajaram Purushottam",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Evolution of Dst and auroral indices during some severe
geomagnetic storms",
journal = "Revista Brasileira de Geof{\'{\i}}sica",
year = "2009",
volume = "27",
number = "2",
pages = "151--163",
keywords = "Dst geomagn{\'e}tico, {\'{\i}}ndices aurorais, tempestades
geomagn{\'e}ticas, geomagnetic Dst, auroral indices, geomagnetic
disturbances.",
abstract = "As evolu{\c{c}}{\~o}es dos {\'{\i}}ndices Dst
geomagn{\'e}tico e AU, AL e AE da aurora foram investigadas em
rela{\c{c}}{\~a}o aos par{\^a}metros interplanet{\'a}rios de
treze tempestades (com {\'{\i}}ndices Dst maiores que 250 nT),
no per{\'{\i}}odo entre 1980 e 2003. As mudan{\c{c}}as no
{\'{\i}}ndice Dst ocorreram toda vez que a componente Bz do
campo B magn{\'e}tico interplanet{\'a}rio se tornou negativa.
Entre os {\'{\i}}ndices da aurora, as mudan{\c{c}}as do
{\'{\i}}ndice AU (representando o eletrojato da aurora em
dire{\c{c}}{\~a}o ao leste) geralmente foram bem menores do que
as do AL (representando o eletrojato da aurora para oeste). Ambos
iniciaram um incremento quase que simultaneamente com o aumento do
campo B magn{\'e}tico interplanet{\'a}rio, muito embora n{\~a}o
tendo, {\`a}s vezes, a componente Bz se tornado negativa.
Portanto, as mudan{\c{c}}as observadas em AU e AL podem preceder
as da Dst por algumas horas e com isso t{\^e}m o potencial de
previs{\~a}o de mudan{\c{c}}a. As mudan{\c{c}}as em AU e AL
n{\~a}o se comportaram em paralelo e as suas
inter-correla{\c{c}}{\~o}es foram quase nulas. Quando Bz se
tornava negativa, invariavelmente AL era alto, por{\'e}m o
reverso n{\~a}o se realizava. Grandes mudan{\c{c}}as em AL
poderiam ocorrer mesmo quando Bz n{\~a}o fosse negativa (ou mesmo
positiva). Valores de AL apresentaram muitos picos durante as
tempestades e invariavelmente estes n{\~a}o se relacionaram
{\`a}s mudan{\c{c}}as de Bz. Picos sucessivos de AL mostraram
separa{\c{c}}{\~o}es em largas faixas, entre 40 e 160 minutos.
An{\'a}lise espectral de valores hor{\'a}rios mostraram
freq{\"u}entes periodicidades ao redor de 2-4 horas, 6 horas e
8-9 horas. ABSTRACT: The evolutions of the geomagnetic Dst and
auroral indices AU, AL, AE were examined in relation to
interplanetary parameters for thirteen severe storms (Dst change
exceeding 250 nT) during 1980-2003. Dst changes occurred every
time Bz component of interplanetary magnetic field B turned
negative. Among the auroral indices, changes in AU (representing
an eastward auroral electrojet) were generally much smaller than
changes in AL (representing a westward auroral electrojet), and
both started increasing almost simultaneously with increases of
interplanetary magnetic field B, even though its Bz component may
not have turned negative. Hence AU and AL changes may precede Dst
changes by a few hours and could have a prediction potential. AU
and AL changes were not correlated well with each other; their
inter-correlation was almost zero. Whenever Bz was negative, AL
indices were invariably high, but the reverse was not true. Large
AL changes could occur even when Bz was not negative (or even when
positive). AL values showed many peaks during the storm and these
were not invariably related to Bz changes. Successive AL peaks had
separations in a wide range of 40-160 minutes. Spectral analysis
of hourly values showed frequent periodicities around 2-4 hours, 6
hours, and 8-9 hours.",
doi = "10.1590/S0102-261X2009000200001",
url = "http://dx.doi.org/10.1590/S0102-261X2009000200001",
issn = "0102-261X",
language = "en",
targetfile = "a01v27n2.pdf",
url = "http://dx.doi.org/10.1590/S0102-261X2009000200001",
urlaccessdate = "15 jun. 2024"
}