@InProceedings{DalLagoBragMesqMend:2018:CoMaEj,
author = "Dal Lago, Alisson and Braga, Carlos Roberto and Mesquita, Amanda
L{\'u}cia and Mendon{\c{c}}a, Rafael Rodrigues Souza de",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)}",
title = "Coronal mass ejection properties at earth’s vicinity",
year = "2018",
organization = "Cospar Scientific Assembly, 42.",
abstract = "It has been now over 20 years of nearly continuous coverage of
solar coronagraphs and interplanetary monitors in the near Earth
space. Several studies have addressed the challenge of predicting
interplanetary disturbance parameters from solar observations.
Special attention has been given to the coronal mass ejections
(CMEs) because they are among the main origins of geomagnetic
disturbances. They change the properties of the near-earth
interplanetary medium, enhancing some key parameters, such as the
southward interplanetary magnetic field and the solar wind speed.
These quantities are known to be related to the energy transfer
from the solar wind to the Earths magnetosphere via the magnetic
reconnection process. Among the several attempts to establish
correlations between CMEs and their interplanetary counterpart
(ICME) properties, it was found that the average CME propagation
speed to 1AU is highly correlated to the ICME peak speed (Dal Lago
et al, 2004). In this work, we present an extended study of such
correlation, which confirms the results found in our previous
study.",
conference-location = "Pasadena, California",
conference-year = "14-22 July",
language = "en",
targetfile = "dal lago_coronal.pdf",
urlaccessdate = "19 abr. 2024"
}