A Space weather information service based upon remote and in-situ measurements of coronal mass ejections heading for Earth

A Space weather information service based upon remote and in-situ measurements of coronal mass ejections heading for Earth

The Earth’s magnetosphere is formed as a consequence of interaction between the planet’s magnetic field and the solar wind, a continuous plasma stream from the Sun. A number of different solar wind phenomena have been studied over the past 40 years with the intention of understanding and forecasting...

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Bibliographic Details
Main Authors: Ritter Birgit, Meskers Arjan J. H., Miles Oscar, Rußwurm Michael, Scully Stephen, Roldán Andrés, Hartkorn Oliver, Jüstel Peter, Réville Victor, Lupu Sorina, Ruffenach Alexis
Format: Article
Language:English
Published: EDP Sciences 2015-01-01
Series:Journal of Space Weather and Space Climate
Subjects:
Coronal Mass Ejection (CME)
Remote sensing
In-situ measurement
Geomagnetic storms
Forecast
Services
Online Access:http://dx.doi.org/10.1051/swsc/2015006

Internet

http://dx.doi.org/10.1051/swsc/2015006

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