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II' Plasma Physics Fundamentals

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Title: II' Plasma Physics Fundamentals


1
II. Plasma Physics Fundamentals
  • 4. The Particle Picture
  • 5. The Kinetic Theory
  • 6. The Fluid Description of Plasmas
  • 7. Waves in Plasma

2
7. Waves in Plasmas
  • 7.1 Electrostatic Waves in Non-Magnetized
  • Plasmas
  • 7.2 Electrostatic Waves in Magnetized Plasmas
  • 7.3 Electromagnetic Waves in Plasmas

3
7.3 Electromagnetic Waves in Plasmas
  • 7.3.1 Electromagnetic Waves Refresher
  • 7.3.2 E.M. Waves in a Non-Magnetized Plasma
  • 7.3.3 E.M. Waves in a Magnetized Plasma
  • 7.3.4 Hydromagnetic (Alfven) Waves
  • 7.3.5 Magnetosonic Waves

4
7.3.1 Electromagnetic Waves Refresher
  • The equation for the e.m. waves can be deducted
    from the Maxwell equations by taking the curl of
    Amperes law in vacuum (j0)
  • Since div H0 and substituting the curl E with
    the Faradays law it is found

5
Electromagnetic Waves Refresher (II)
  • The vector H then satisfies the Helmholtz wave
    equation
  • In a perfectly similar fashion it can be derived
    a wave equation for E
  • It can be verified by substitution that a
    solution of the Helmholtz equation is
    exp(ikx-iwt) for w/kc

6
Electromagnetic Waves Refresher (III)
  • The electromagnetic field E, H propagates in
    vacuum with phase velocity w/kc
  • The relation w/kc constitutes the dispersion
    relation for electromagnetic waves in vacuum
  • Since the e.m. field of the wave must satisfy the
    Maxwell equations and r0 (in vacuum there are no
    charges), if Ew is the vector of wave electric
    field amplitude, it will be (for k along the x
    axis)

that implies
7
Electromagnetic Waves Refresher (IV)
  • The electric field of an e.m. wave then must not
    have a component along the propagation direction
    k (must be perpendicular to k)
  • By taking the curl of the electric field
    component of the wave and using Faradays law it
    can be easily shown that the magnetic field also
    lies in a plane perpendicular to k ( and
    direction perpendicular to both k and E)

8
7.3.2 Electromagnetic Waves in a Plasma
  • In a plasma there will be current carriers,
    therefore the curl of Amperes law is
  • By taking the curl of Faradays law

and eliminating the curl of H
9
Electromagnetic Waves in a Plasma (II)
  • If a wave solution of the form exp(kr-wt) is
    assumed it can be written (De0E)
  • By recalling that an e.m. must be transverse (kE
    0) and that c21/(m0e0) it follows
  • In order to estimate the current the ions are
    considered fixed (good approximation for high
    frequencies) and the current is carried by
    electrons with density n0 and velocity u

10
Electromagnetic Waves in a Plasma (III)
  • The electron equation of motion is
  • The motion of the electrons here is the
    self-consistent solution of u, E, B (E and B are
    not external imposed field like in the particle
    trajectory calculations)
  • A first-order form of the equation of motion is
    then

then
11
Electromagnetic Waves in a Plasma (IV)
  • Finally, substituting the expression of j in

it is found
  • that is the dispersion relation for e.m. waves
    in a plasma (without external magnetic field)
  • The phase velocity is always greater than c while
    the group velocity is always less than c

12
Electromagnetic Waves in a Plasma (V)
  • For a given frequency w the dispersion relation
  • gives a particular k or wavelength (k2p/l) for
    the wave propagation
  • If the frequency is raised up to wwp then it
    must be k0. This is the cutoff frequency
    (conversely, cutoff densitywill be the value that
    makes wp equal to w)
  • For even larger densities, or simply wltwp there
    is no real k that satisfies the dispersion
    relation and the wave cannot propagate through
    the plasma

13
Electromagnetic Waves in a Plasma (VI)
  • When k becomes imaginary the wave is attenuated
  • The spatial part of the wave can be written as

where d is the skin depth defined as
14
7.3.3 E.M. Waves in a Magnetized Plasma
  • The case of an e.m. wave perpendicular to an
    external magnetic field B0 is considered
  • If the wave electric field is parallel to B0 the
    same derivation as for non magnetized plasma can
    be applied (essentially because the first-order
    electron equation of motion is not affected by
    B0)
  • The the wave is called ordinary wave and the
    dispersion relation in this case is still

z
E
B0
k
y
x
15
E.M. Waves in a Magnetized Plasma (II)
  • The case of the wave electric field perpendicular
    to B0 requires both x and y components of E since
    the wave becomes elliptically polarized

z
E
B0
k
y
x
  • A linearized (first-order) form of the equation
    electron equation of motion is then

16
E.M. Waves in a Magnetized Plasma (III)
  • The wave equation now must keep the longitudinal
    electric field kEkEx

or
  • By solving for the separate x and y components a
    dispersion relation for the extraordinary wave is
    found as

17
E.M. Waves in a Magnetized Plasma (IV)
  • The case of the wave vector parallel to B0 also
    requires both x and y components of E

z
k
E
B0
y
x
  • The same derivation as for the extraordinary wave
    can be used by simply by changing the direction
    of k

18
E.M. Waves in a Magnetized Plasma (V)
  • The resulting dispersion relation is
  • or the choice of sign distinguish between a
    right-hand circular polarization (R-wave) and a
    left hand circular polarization (L-wave)
  • The R-wave has a resonance corresponding to the
    electron Larmor frequency in this case the wave
    looses energy by accelerating the electrons along
    the Larmor orbit
  • It can be shown that the L-wave has a resonance
    in correspondence to the ion Larmor frequency

19
7.3.4 Hydromagnetic (Alfven) Waves
  • This case considers still the wave vector
    parallel to B0 but includes both electrons and
    ion motions and current j and electric field E
    perpendicular to B0

z
k
B0
E,j
y
x
  • The solution neglects the electron Larmor orbits,
    leaving only the ExB drift and considers
    propagation frequencies much smaller than the ion
    cyclotron frequency

20
Hydromagnetic (Alfven) Waves (II)
  • The dispersion relation for the hydromagnetic
    (Alfven) waves can be derived as
  • where r is the mass density
  • It can be shown that the denominator is the
    relative dielectric constant for low-frequency
    perpendicular motion in the plasma
  • The dispersion relation for Alfven waves gives
    the phase velocity of e.m. waves in the plasma
    considered as a dielectric medium

21
Hydromagnetic (Alfven) Waves (III)
  • In most laboratory plasmas the dielectric
    constant is much larger than unity, therefore,
    for hydromagnetic waves,
  • where vA is the Alfven velocity
  • The Alfven velocity can be considered the
    velocity of the perturbations of the magnetic
    lines of force due to the wave magnetic field in
    the plasma
  • Under the approximations made the fluid and the
    field lines oscillate as they were glued
    together

22
7.3.5 Magnetosonic Waves
  • This case considers the wave vector perpendicular
    to B0 and includes both electrons and ion motions
    (low-frequency waves) with E perpendicular to B0

z
k
B0
E
y
x
  • The solution includes the pressure gradient in
    the (fluid) equation of motion since the
    oscillating ExB0 drifts will cause compressions
    in the direction of the wave

23
Magnetosonic Waves (II)
  • For frequencies much smaller than the ion
    cyclotron frequency the dispersion relation for
    magnetosonic waves can be derived as
  • where vs is the sound speed in the plasma
  • The magnetosonic wave is an ion-acoustic wave
    that travels perpendicular to the magnetic field
  • Compressions and rarefactions are due to the ExB0
    drifts

24
Magnetosonic Waves (III)
  • In the limit of zero magnetic field the
    ion-acoustic dispersion relation is recovered
  • In the limit of zero temperature the sound speed
    goes to zero and the wave becomes similar to an
    Alfven wave
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