Charged particle reflection in a magnetic mirror

Authors

  • Luis Ángel Fernández Instituto Nacional de Astrofísica, Óptica y Electrónica
  • José Eduardo Mendoza Torres Instituto Nacional de Astrofísica, Óptica y Electrónica
  • Octavio Gomez Flores Instituto Nacional de Astrofísica, Óptica y Electrónica
  • Eduardo Tirado Bueno Instituto Nacional de Astrofísica, Óptica y Electrónica

DOI:

https://doi.org/10.31349/RevMexFisE.21.020211

Keywords:

Magnetic Mirror, Monte Carlo, Plasma

Abstract

We study the reflection of electrons in a magnetic field mirror. It is a field with a gradient from a lowest value B0 to a largest one Bm. With this purpose, Montecarlo simulations are made. We use a number of 5,000 particles with random pitch angles. The frequency distribution of these random values follows a Gaussian distribution centered at  \theta = 0 and with standard deviation \sigma. Various values of \sigma and also different values of the B0 /Bm ratio are used in the simulations. The simulations show that \sigma has an important influence on the confinement of charged particles, for the different B0 /Bm ratios here studied. However, the percent of reflected particles differs from a B0 /Bm ratio to another in the whole range of \sigma, although for \sigma = 10 the differences between different ratios are small (<5%). The number of reflected particles increases very rapidly with \sigma, in the range of 10° to 40°. For the \sigma range from 20° to 40°, the percent of reflected particles is \leq 20% larger for B0 /Bm = 0.10 than for the 0.55 ratio.

References

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R. H. Goddard, (Clark University Archive)

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Published

2024-07-01

How to Cite

[1]
L. Ángel Fernández, J. E. . Mendoza Torres, O. . Gomez Flores, and E. Tirado Bueno, “Charged particle reflection in a magnetic mirror”, Rev. Mex. Fis. E, vol. 21, no. 2 Jul-Dec, pp. 020211 1–, Jul. 2024.