@InProceedings{Gonzalez-AlarconTsur:1992:GeStRe,
author = "Gonzalez-Alarcon, Walter Demetrio and Tsurutani, B. T.",
title = "Terrestrial response to eruptive solar flares: geomagnetic storms:
a review",
year = "1992",
pages = "277--286",
organization = "Frontiers in Physics: Eruptive Solar Flares.",
publisher = "Springer Verlag",
keywords = "GEOFISICA ESPACIAL, TEMPESTADE MAGNETICA, ERUPCAO.",
abstract = "During the interval of August 1978 - December 1979, 56 unambiguous
fast forward shocks were identified using magnetic field and
plasma data collected by the ISEE-3 spacecraft. Because this
interval is at a solar maximum we assume the streams causing these
shocks are associated with coronal mass ejections and eruptive
solar flares. For these shocks we shall describe the shock- storm
relationship for the level of intense storms (Dst < -100 nT).
Then, we will discuss the interplanetary structures that are
associated with the large-amplitude and long-duration negative B,
fields,which are found in the sheath field and/or driver gas
regions of the shock and are thought to be the main cause of the
intense storms. We will also present for the solar physicist a
summary of the interplanetary/magnetosphere coupling functions,
based on the magnetopause reconnection process. We will end by
giving an overview of the long-term evolution of geornagnetic
storms such as those associated with the seasonal and solar cyle
distributions.",
conference-year = "1992",
label = "8678",
targetfile = "gonzalez_terrestrial.pdf",
urlaccessdate = "29 jun. 2024"
}