Contains fulltext : 159664.pdf (preprint version ) (Open Access
Contains fulltext : 161145.pdf (preprint version ) (Open Access)5 p
[[abstract]]We use the Time History of Events and Macroscale Interactions during Substorms data to i...
The current state of the art in the modeling of pulsar magnetospheres invokes either the vacuum or f...
Contains fulltext : 150890.pdf (preprint version ) (Open Access
Contains fulltext : 132497.pdf (preprint version ) (Open Access
Contains fulltext : 111263.pdf (preprint version ) (Closed access
Contains fulltext : 178657.pdf (publisher's version ) (Closed access) ...
Context. Eruption of a coronal mass ejection (CME) drags and "opens" the coronal magnetic field, pre...
Contains fulltext : 92721.pdf (publisher's version ) (Open Access
Magnetars may have a strong surface dipole field. Observationally, two magnetars may have passive fa...
The following full text is a publisher's version. For additional information about this publica...
The canonical pulsar magnetosphere contains a bubble of closed magnetic field lines that is separate...
International audienceDuring the first year of the Magnetospheric Multiscale Mission (MMS) there hav...
Over the past three decades, terrestrial magnetospheric physics has had a unifying and hotly debated...
Contains fulltext : 91272.pdf (publisher's version ) (Open Access
Contains fulltext : 161145.pdf (preprint version ) (Open Access)5 p
[[abstract]]We use the Time History of Events and Macroscale Interactions during Substorms data to i...
The current state of the art in the modeling of pulsar magnetospheres invokes either the vacuum or f...
Contains fulltext : 150890.pdf (preprint version ) (Open Access
Contains fulltext : 132497.pdf (preprint version ) (Open Access
Contains fulltext : 111263.pdf (preprint version ) (Closed access
Contains fulltext : 178657.pdf (publisher's version ) (Closed access) ...
Context. Eruption of a coronal mass ejection (CME) drags and "opens" the coronal magnetic field, pre...
Contains fulltext : 92721.pdf (publisher's version ) (Open Access
Magnetars may have a strong surface dipole field. Observationally, two magnetars may have passive fa...
The following full text is a publisher's version. For additional information about this publica...
The canonical pulsar magnetosphere contains a bubble of closed magnetic field lines that is separate...
International audienceDuring the first year of the Magnetospheric Multiscale Mission (MMS) there hav...
Over the past three decades, terrestrial magnetospheric physics has had a unifying and hotly debated...
Contains fulltext : 91272.pdf (publisher's version ) (Open Access
Contains fulltext : 161145.pdf (preprint version ) (Open Access)5 p
[[abstract]]We use the Time History of Events and Macroscale Interactions during Substorms data to i...
The current state of the art in the modeling of pulsar magnetospheres invokes either the vacuum or f...