%0 Journal Article %1 HeliEvent %A Hietala, H. %A Sandroos, A. %A Vainio, R. %D 2012 %J The Astrophysical Journal Letters %K acceleration bow magnetosphere particle shock %N 1 %P L14 %T Particle Acceleration in Shock–Shock Interaction: Model to Data Comparison %U http://stacks.iop.org/2041-8205/751/i=1/a=L14 %V 751 %X Shock-shock interaction is a well-established particle acceleration mechanism in astrophysical and space plasmas, but difficult to study observationally. Recently, the interplanetary shock collision with the bow shock of the Earth on 1998 August 10 was identified as one of the rare events where detailed in situ observations of the different acceleration phases can be made. Due to the advantageous spacecraft and magnetic field configurations, in 2011, Hietala et al. were able to distinguish the seed population and its reacceleration at the bow shock, as well as the Fermi acceleration of particles trapped between the shocks. They also interpreted their results as being the first in situ evidence of the release of particles from the trap as the two shocks collided. In the present study we use a global 2.5D test-particle simulation to further study particle acceleration in this event. We concentrate on the last phases of the shock-shock interaction, when the shocks approach and pass through each other. The simulation results verify that the main features of the measurements can be explained by shock-shock interaction in this magnetic geometry, and are in agreement with the previous interpretation of particle release. Shock-shock collisions of this type occur commonly in many astrophysical locations such as stellar coronae, planetary and cometary bow shocks, and the distant heliosphere.

@article{HeliEvent, abstract = {Shock-shock interaction is a well-established particle acceleration mechanism in astrophysical and space plasmas, but difficult to study observationally. Recently, the interplanetary shock collision with the bow shock of the Earth on 1998 August 10 was identified as one of the rare events where detailed in situ observations of the different acceleration phases can be made. Due to the advantageous spacecraft and magnetic field configurations, in 2011, Hietala et al. were able to distinguish the seed population and its reacceleration at the bow shock, as well as the Fermi acceleration of particles trapped between the shocks. They also interpreted their results as being the first in situ evidence of the release of particles from the trap as the two shocks collided. In the present study we use a global 2.5D test-particle simulation to further study particle acceleration in this event. We concentrate on the last phases of the shock-shock interaction, when the shocks approach and pass through each other. The simulation results verify that the main features of the measurements can be explained by shock-shock interaction in this magnetic geometry, and are in agreement with the previous interpretation of particle release. Shock-shock collisions of this type occur commonly in many astrophysical locations such as stellar coronae, planetary and cometary bow shocks, and the distant heliosphere.}, added-at = {2013-02-27T14:19:43.000+0100}, author = {Hietala, H. and Sandroos, A. and Vainio, R.}, biburl = {https://www.bibsonomy.org/bibtex/2d61280e8af9cf8d33a79536f53cef77a/ursg}, description = {Particle Acceleration in Shock–Shock Interaction: Model to Data Comparison - Abstract - The Astrophysical Journal Letters - IOPscience}, interhash = {1461ce37d71736127e647cfada3f611f}, intrahash = {d61280e8af9cf8d33a79536f53cef77a}, journal = {The Astrophysical Journal Letters}, keywords = {acceleration bow magnetosphere particle shock}, number = 1, pages = {L14}, timestamp = {2013-02-27T14:19:43.000+0100}, title = {Particle Acceleration in Shock–Shock Interaction: Model to Data Comparison}, url = {http://stacks.iop.org/2041-8205/751/i=1/a=L14}, volume = 751, year = 2012 }