Magnetic mirrors / Fermi acceleration

Fonte: My Solutions
Revisão em 17h25min de 14 de junho de 2017 por Ist426982 (discussão | contribs)
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(F. F. Chen ~ 2.12, Fermi acceleration of cosmic rays).

A cosmic ray proton is trapped between two moving magnetic mirrors with mirror ratio \(R_m=5\). Initially its energy is $W=1$ keV and $v_\perp = v_\parallel$ at the midplane. Each mirror moves toward the midplane with a velocity $v_m=10$ km/s and the initial distance between the mirrors is $L=10^{10}$ km.