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Physics · 术语表

什么是 Plasma; the free-electron model?

Definition 14.1 University Physics — Year 2 · 第 14 章 — Electromagnetic Waves in Plasmas, Conductors and Dielectrics

A plasma is a globally neutral gas of free electrons (density nn, mass mm, charge −e-e) and positive ions, which, being thousands of times heavier, are taken as fixed. The upper atmosphere (ionosphere, n∼1011n \sim 10^{11}–101210^{12} m−3^{-3}), a discharge tube, the solar corona, and — at optical frequencies — the conduction electrons of a metal are plasmas. Collisions are neglected (the wave’s period is short compared with the time between collisions). Its characteristic frequency is the plasma frequency

ωp=ne2ε0m,fp=ωp2π≈9 Hz×n [m−3]:\omega_p = \sqrt{\frac{ne^2}{\varepsilon_0m}} , \qquad f_p = \frac{\omega_p}{2\pi} \approx 9\,\text{Hz}\times\sqrt{n\,[\text{m}^{-3}]} :

3 MHz3\,\mathrm{MHz} to 9 MHz9\,\mathrm{MHz} for the ionosphere, 2×1015 Hz2 \times 10^{15}\,\mathrm{Hz} (ultraviolet) for a metal.

Left: the dispersion relation of a plasma — no propagation below _p, a hyperbola approaching the light line above. Right: shortwaves below the plasma frequency are reflected by the ionosphere and hop around the Earth; higher frequencies escape to space. Left: the dispersion relation of a plasma — no propagation below _p, a hyperbola approaching the light line above. Right: shortwaves below the plasma frequency are reflected by the ionosphere and hop around the Earth; higher frequencies escape to space.
Left: the dispersion relation of a plasma — no propagation below ωp\omega_p, a hyperbola approaching the light line above. Right: shortwaves below the plasma frequency are reflected by the ionosphere and hop around the Earth; higher frequencies escape to space.

示例

Example 14.4 (The ionosphere and radio)

With n=1×1012 m−3n = 1 \times 10^{12}\,\mathrm{m}^{-3} in the F layer, fp=9 MHzf_p = 9\,\mathrm{MHz}: shortwave broadcasts below that are reflected (and can hop around the Earth between the ionosphere and the ground), FM (100 MHz100\,\mathrm{MHz}), television and satellite links pass through. A wave at 3 MHz3\,\mathrm{MHz} penetrates only 1/κ=c/ωp2−ω2=6 m1/\kappa = c/\sqrt{\omega_p^2 - \omega^2} = 6\,\mathrm{m} into the layer before turning back. A spacecraft re-entering the atmosphere is sheathed in a plasma of n∼1018n \sim 10^{18} m−3^{-3}, fp∼10 GHzf_p \sim 10\,\mathrm{GHz}: radio contact is lost for minutes.

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