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Pursuing Forecasts of the Behavior and Arrival of Coronal Mass Ejections through Modeling and Observations

Published online by Cambridge University Press:  24 July 2018

Hebe Cremades
Hebe Cremades*
Affiliation:
Universidad Tecnológica Nacional – Facultad Regional Mendoza, CEDS Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET) Rodríguez 243, 5500, Mendoza, Argentina email: hebe.cremades@frm.utn.edu.ar
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Abstract

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Sophisticated instrumentation dedicated to studying and monitoring our Sun’s activity has proliferated in the past few decades, together with the increasing demand of specialized space weather forecasts that address the needs of commercial and government systems. As a result, theoretical and empirical models and techniques of increasing complexity have been developed, aimed at forecasting the occurrence of solar disturbances, their evolution, and time of arrival to Earth. Here we will review groundbreaking and recent methods to predict the propagation and evolution of coronal mass ejections and their driven shocks. The methods rely on a wealth of data sets provided by ground- and space-based observatories, involving remote-sensing observations of the corona and the heliosphere, as well as detections of radio waves.

Keywords

Sun: coronal mass ejections (CMEs)solar-terrestrial relationsinterplanetary medium
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S335: Space Weather of the Heliosphere: Processes and Forecasts , July 2017 , pp. 58 - 64
Copyright
Copyright © International Astronomical Union 2018 

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