Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/94695/1/jgra21551.pd
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/99630/1/jgra50428.pd
Energetic electrons are a common feature of interplanetary shocks and planetary bow shocks, and they...
Collisionless shocks are some of the most efficient particle accelerators in heliospheric and astrop...
Collisionless shock waves are a widespread phenomenon in both solar system and astrophysical context...
Shock waves are widespread in collisionless space plasmas throughout the Universe. How particles are...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95313/1/jgra21189.pd
Collisionless shocks vary drastically from terrestrial to astrophysical regimes resulting in radical...
The leading explanation for the origin of galactic cosmic rays is particle acceleration at the shock...
Shock waves exist throughout the universe and are fundamental to understanding the nature of collisi...
During periods of high solar wind pressure, Saturn's bow shock is pushed inside Titan's orbit exposi...
Astrophysical shocks, such as planetary bow shocks or supernova remnant shocks, are often in the hig...
International audienceElectrons can be accelerated to ultrarelativistic energies at strong (high-Mac...
Shock waves form when supersonic flows encounter an obstacle. Like in regular gases, shock waves can...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/99630/1/jgra50428.pd
Energetic electrons are a common feature of interplanetary shocks and planetary bow shocks, and they...
Collisionless shocks are some of the most efficient particle accelerators in heliospheric and astrop...
Collisionless shock waves are a widespread phenomenon in both solar system and astrophysical context...
Shock waves are widespread in collisionless space plasmas throughout the Universe. How particles are...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95313/1/jgra21189.pd
Collisionless shocks vary drastically from terrestrial to astrophysical regimes resulting in radical...
The leading explanation for the origin of galactic cosmic rays is particle acceleration at the shock...
Shock waves exist throughout the universe and are fundamental to understanding the nature of collisi...
During periods of high solar wind pressure, Saturn's bow shock is pushed inside Titan's orbit exposi...
Astrophysical shocks, such as planetary bow shocks or supernova remnant shocks, are often in the hig...
International audienceElectrons can be accelerated to ultrarelativistic energies at strong (high-Mac...
Shock waves form when supersonic flows encounter an obstacle. Like in regular gases, shock waves can...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/99630/1/jgra50428.pd
Energetic electrons are a common feature of interplanetary shocks and planetary bow shocks, and they...
Collisionless shocks are some of the most efficient particle accelerators in heliospheric and astrop...
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