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 foreca...
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: | |
Online Access: | http://dx.doi.org/10.1051/swsc/2015006 |
Similar Items
-
Analytical and empirical modelling of the origin and heliospheric propagation of coronal mass ejections, and space weather applications
by: Vršnak Bojan
Published: (2021-01-01) -
Geometry of Coronal Mass Ejections in the Context of Recent Solar Cycle
by: Mishra Rajesh, et al.
Published: (2010-01-01) -
Halo coronal mass ejections during Solar Cycle 24: reconstruction of the global scenario and geoeffectiveness
by: Scolini Camilla, et al.
Published: (2018-01-01) -
Characteristics of Magnetic Clouds and Interplanetary Coronal Mass Ejections which Cause Intense Geomagnetic Storms
by: Chin-Chun Wu, et al.
Published: (2013-01-01) -
Investigating the kinematics of coronal mass ejections with the automated CORIMP catalog
by: Byrne Jason P.
Published: (2015-01-01)