Field-aligned diffusion of energetic ions in the Earth’s foreshock is investigated by using the quasi-linear theory (QLT)and test particle simulation
The foreshock region is located upstream of the terrestrial bow shock and is characterized by energe...
International audienceThe ion foreshock located upstream of the Earth's shock front is populated wit...
International audienceThe ion foreshock located upstream of the Earth's bow shock is populated with ...
This study reports observations of energetic ions upstream of the Earth’s quasi-parallel bow shock b...
International audienceThis study reports observations of energetic ions upstream of the Earth’s quas...
International audienceWe study parallel (field-aligned) diffusion of energetic particles in the upst...
European Research Council Starting grant (200141-QuESpace). Grant Number: ST/K001051/1; German Resea...
International audienceField-aligned beams are known to originate from the quasi-perpendicular side o...
The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow...
We study the solar wind interaction with Mars in a global three-dimensional hybrid model. A well-dev...
International audienceCollisionless shocks are well-known structures in astrophysical environments w...
The foreshock region is located upstream of the terrestrial bow shock and is characterized by energe...
International audienceThe ion foreshock located upstream of the Earth's shock front is populated wit...
International audienceThe ion foreshock located upstream of the Earth's bow shock is populated with ...
This study reports observations of energetic ions upstream of the Earth’s quasi-parallel bow shock b...
International audienceThis study reports observations of energetic ions upstream of the Earth’s quas...
International audienceWe study parallel (field-aligned) diffusion of energetic particles in the upst...
European Research Council Starting grant (200141-QuESpace). Grant Number: ST/K001051/1; German Resea...
International audienceField-aligned beams are known to originate from the quasi-perpendicular side o...
The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow...
We study the solar wind interaction with Mars in a global three-dimensional hybrid model. A well-dev...
International audienceCollisionless shocks are well-known structures in astrophysical environments w...
The foreshock region is located upstream of the terrestrial bow shock and is characterized by energe...
International audienceThe ion foreshock located upstream of the Earth's shock front is populated wit...
International audienceThe ion foreshock located upstream of the Earth's bow shock is populated with ...
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