TY - JOUR
T1 - Scattering of Superthermal Ions at Shocks
T2 - Dependence on Energy
AU - Gedalin, Michael
AU - Ganushkina, Natalia
AU - Pogorelov, Nikolai V.
AU - Roytershteyn, Vadim
N1 - Publisher Copyright:
© 2023. The Author(s). Published by the American Astronomical Society.
PY - 2023/11/1
Y1 - 2023/11/1
N2 - Diffusive shock acceleration requires the production of backstreaming superthermal ions (injection) as a first step. Such ions can be generated in the process of scattering of ions in the superthermal tail off the shock front. Knowledge of the scattering of high-energy ions is essential for matching conditions of upstream and downstream distributions at the shock transition. Here we analyze the generation of backstreaming ions as a function of their initial energy in a model stationary shock and in a similar rippled shock. Rippling substantially enhances ion reflection and the generation of backstreaming ions for slightly and moderately superthermal energies, and thus is capable of ensuring ion injection into a further diffusive shock acceleration process. For high-energy ions, there is almost no difference in the fraction of backstreaming ions produced and the ion distributions between the planar stationary shock and the rippled shock.
AB - Diffusive shock acceleration requires the production of backstreaming superthermal ions (injection) as a first step. Such ions can be generated in the process of scattering of ions in the superthermal tail off the shock front. Knowledge of the scattering of high-energy ions is essential for matching conditions of upstream and downstream distributions at the shock transition. Here we analyze the generation of backstreaming ions as a function of their initial energy in a model stationary shock and in a similar rippled shock. Rippling substantially enhances ion reflection and the generation of backstreaming ions for slightly and moderately superthermal energies, and thus is capable of ensuring ion injection into a further diffusive shock acceleration process. For high-energy ions, there is almost no difference in the fraction of backstreaming ions produced and the ion distributions between the planar stationary shock and the rippled shock.
UR - http://www.scopus.com/inward/record.url?scp=85176926269&partnerID=8YFLogxK
U2 - 10.3847/1538-4357/ad04dd
DO - 10.3847/1538-4357/ad04dd
M3 - Article
AN - SCOPUS:85176926269
SN - 0004-637X
VL - 957
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
M1 - 106
ER -