@Article{AlarconEche:2005:StPeDs,
author = "Alarcon, Walter Dem{\'e}trio Gonzalez and Echer, Ezequiel",
affiliation = "Instituto Nacional de Pesquisas Espaciais, Divis{\~a}o de
Geof{\'{\i}}sica Espacial (INPE, DGE)",
title = "A study on the peak Dst and peak negative Bz relationship during
intense geomagnetic storms",
journal = "Geophysical Research Letters",
year = "2005",
volume = "32",
number = "8",
month = "Sept.",
abstract = "This paper is a study of the relationship between the geomagnetic
storm index Dst and the southward component, Bs, of the
interplanetary magnetic field (IMF) driver. This study was
performed during the ACE observational period (1997-2002), for
which 64 intense geomagnetic storms (Dst <= -85 nT) were analyzed.
After taking into account the propagation time between the L1
point and Earth (similar to 1 h) and the magnetosphere/ring
current response-time to solar wind forcing (similar to 1 h), it
was determined that the average delay between the peak Bs and the
peak Dst values is similar to 2 h. It was also observed that the
Bs value at peak Dst is similar to 75% of the peak Bs value in the
entire event. When these results are analyzed in terms of the
interplanetary electric field, associated with Bz, some
interesting additional studies are indicated, for which some
simple results, of practical space weather forecasting use, are
anticipated.",
copyholder = "SID/SCD",
issn = "0094-8276",
language = "en",
targetfile = "a study on the peak Dst, gonzalez.pdf",
urlaccessdate = "15 jun. 2024"
}