Diferenças entre edições de "Magnetic mirrors / Fermi acceleration"
| (Há uma edição intermédia do mesmo utilizador que não está a ser apresentada) | |||
| Linha 7: | Linha 7: | ||
(a) Using the invariance of \(\mu\), find the energy to which the proton is accelerated before it escapes. | (a) Using the invariance of \(\mu\), find the energy to which the proton is accelerated before it escapes. | ||
| − | (b) How long does it take to reach that energy? Suggestions: i) suppose that the | + | (b) How long does it take to reach that energy? Suggestions: i) suppose that the \(B\) field is approxiamtely uniform in the space between the mirrors and changes abruptly near the mirrors, ''i.e.'', treat each mirror as a flat piston and show that the velocity gained at each bounce is \(2v_m\); ii) compute the number of bounces necessary; iii) assume that the distance between the mirrors does not change appreciably |
during the acceleration process. | during the acceleration process. | ||
Edição atual desde as 16h53min de 17 de junho de 2017
(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.
(a) Using the invariance of \(\mu\), find the energy to which the proton is accelerated before it escapes.
(b) How long does it take to reach that energy? Suggestions: i) suppose that the \(B\) field is approxiamtely uniform in the space between the mirrors and changes abruptly near the mirrors, i.e., treat each mirror as a flat piston and show that the velocity gained at each bounce is \(2v_m\); ii) compute the number of bounces necessary; iii) assume that the distance between the mirrors does not change appreciably during the acceleration process.