@InProceedings{DalLagoLGMSVEGES:2006:3dGeCo,
author = "Dal Lago, Alisson and Lucas, Aline de and Gonzalez, Walter
Dem{\'e}trio and McAndrews, H. J. and Schwenn, R. and Vieira,
Luis Eduardo Antunes and Echer, Ezequiel and Guarnieri, Fernando
Luis and Echer, Ezequiel and Silva, Marlos Rockenbach da",
affiliation = "Instituto Nacional de Pesquisas Espaciais, Divis{\~a}o de
Geof{\'{\i}}sica Espacial (INPE.DGE) and Instituto Nacional de
Pesquisas Espaciais, Divis{\~a}o de Geof{\'{\i}}sica Espacial
(INPE.DGE) and Instituto Nacional de Pesquisas Espaciais,
Divis{\~a}o de Geof{\'{\i}}sica Espacial (INPE.DGE) and
{Mullard Space Sciences Laboratory} and {Max-Planck- Institute
fuer Sonnesystemforschung} and Instituto Nacional de Pesquisas
Espaciais, Divis{\~a}o de Geof{\'{\i}}sica Espacial (INPE.DGE)
and Instituto Nacional de Pesquisas Espaciais, Divis{\~a}o de
Geof{\'{\i}}sica Espacial (INPE.DGE) and Instituto Nacional de
Pesquisas Espaciais, Divis{\~a}o de Geof{\'{\i}}sica Espacial
(INPE.DGE) and Instituto Nacional de Pesquisas Espaciais,
Divis{\~a}o de Geof{\'{\i}}sica Espacial (INPE.DGE) and
Instituto Nacional de Pesquisas Espaciais, Divis{\~a}o de
Geof{\'{\i}}sica Espacial (INPE.DGE)",
title = "3d geometry of coronal mass ejections",
booktitle = "Proceedings...",
year = "2006",
organization = "European Geosciences Union (EGU) General Assembly.",
abstract = "Coronal mass ejections are the main source of space weather
disturbances, thus understanding their evolution is a crussial
point for forecasting their impacts at earth. Near the sun, 3
dimentional observations are not available, thus the 3D geometry
of CMEs are still under debate. Based on 2D observational
parameters we investigate the possible 3D geometry of coronal mass
ejections. These parameters are the perpendicular expansion and
the radial expansion. Three cone models are annalized and their
evolution studied. If the geometry of CMEs is known, and if it is
possible to have a similar model for all CMEs, this can be used to
correct and interpret the meaning of the plane-of-sky speeds
measured by coronagraphs like the Large Angle and Spectroscopic
Coronagraph - LASCO, abord the Solar and Heliospheric Observatory
- SOHO. This knowledge would improve subtancially the forecasting
of CME arrival time at earth models.",
conference-location = "Vienna, Austria",
conference-year = "2006-04-02",
language = "en",
urlaccessdate = "03 maio 2024"
}