@Article{GonzálezEcheGonzTsur:2007:InOrIn,
author = "Gonz{\'a}lez, Walter Dem{\'e}trio and Echer, Ezequiel and
Gonz{\'a}lez, Alicia Luiza Cl{\'u}a de and Tsurutani, Bruce T.",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and Jet Propulsion Laboratory,
California Institute of Technology",
title = "Interplanetary origin of intense geomagnetic storms (Dst <-100 nT)
during solar cycle 23",
journal = "Geophysical Research Letters",
year = "2007",
volume = "34",
number = "6",
pages = "1--4",
month = "Mar.",
keywords = "coronal mass ejections, solar-wind, magnetic storms,
geoeffectiveness, geophysics.",
abstract = "We study the interplanetary causes of intense geomagnetic storms
(Dst < -100 nT) that occurred during solar cycle 23 (1997-2005).
It was found that the most common interplanetary structures
leading to the development of an intense storm were: magnetic
clouds, sheath fields, sheath fields followed by a magnetic cloud
and corotating interaction regions leading high speed streams.
However, the relative importance of each of those driving
structures was found to vary with the solar cycle phase. We divide
the cycle in three phases (rising, maximum and declining) and
explain the differences. We also discuss about the
geoeffectiveness of each of the four main interplanetary driving
structures.",
doi = "10.1029/2006GL028879",
url = "http://dx.doi.org/10.1029/2006GL028879",
issn = "0094-8276",
language = "en",
targetfile = "grl22753.pdf",
urlaccessdate = "15 jun. 2024"
}