This study reports observations of energetic ions upstream of the Earth’s quasi-parallel bow shock by Cluster at times when interspacecraft separation distances were larg
International audienceThe ion foreshock located upstream of the Earth's bow shock is populated with ...
It is shown that ions can be accelerated to about 100 keV in the direction perpendicular to the magn...
Beams of Almost Monoenergetic Ions (AMI) in the energy range from 20 to 800 keV were discovered in ...
International audienceThis study reports observations of energetic ions upstream of the Earth’s quas...
International audienceField-aligned beams are known to originate from the quasi-perpendicular side o...
Field-aligned diffusion of energetic ions in the Earth’s foreshock is investigated by using the quas...
Abstract. Field-aligned beams are known to originate from the quasi-perpendicular side of the Earth’...
International audienceA statistical investigation of the location of onset of intermediate and gyrat...
The Earth's bow shock is a boundary where the solar wind becomes decelerated from supersonic to subs...
International audienceThe dynamics of the ion distribution function near the Earth's bow shock is st...
International audienceAn energetic ion (E=40) event observed by the CLUSTER/CIS experiment upstream ...
We present measurements from the ESA/NASA Cluster mission that show in situ acceleration of ions to ...
International audienceWe present a case study of Geotail, Interball-1, IMP-8, and Wind observations ...
The Mars Express Analyzer of Space Plasmas and Energetic Atoms experiment contains ion and electron ...
The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow...
International audienceThe ion foreshock located upstream of the Earth's bow shock is populated with ...
It is shown that ions can be accelerated to about 100 keV in the direction perpendicular to the magn...
Beams of Almost Monoenergetic Ions (AMI) in the energy range from 20 to 800 keV were discovered in ...
International audienceThis study reports observations of energetic ions upstream of the Earth’s quas...
International audienceField-aligned beams are known to originate from the quasi-perpendicular side o...
Field-aligned diffusion of energetic ions in the Earth’s foreshock is investigated by using the quas...
Abstract. Field-aligned beams are known to originate from the quasi-perpendicular side of the Earth’...
International audienceA statistical investigation of the location of onset of intermediate and gyrat...
The Earth's bow shock is a boundary where the solar wind becomes decelerated from supersonic to subs...
International audienceThe dynamics of the ion distribution function near the Earth's bow shock is st...
International audienceAn energetic ion (E=40) event observed by the CLUSTER/CIS experiment upstream ...
We present measurements from the ESA/NASA Cluster mission that show in situ acceleration of ions to ...
International audienceWe present a case study of Geotail, Interball-1, IMP-8, and Wind observations ...
The Mars Express Analyzer of Space Plasmas and Energetic Atoms experiment contains ion and electron ...
The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow...
International audienceThe ion foreshock located upstream of the Earth's bow shock is populated with ...
It is shown that ions can be accelerated to about 100 keV in the direction perpendicular to the magn...
Beams of Almost Monoenergetic Ions (AMI) in the energy range from 20 to 800 keV were discovered in ...