Next: Bibliography
Up: Waves in Warm Plasmas
Previous: Harris Instability
- Derive the dispersion relation (8.28) from Equations (8.23)-(8.27).
- Show that the dispersion relation (8.28) can be written
where
,
,
,
, and
Demonstrate that, in the limit
,
, the approximate solution is
- Show that, when combined with the Maxwellian velocity distribution (8.24), the dispersion relation (8.23) reduces to
where
,
,
, and
is the plasma dispersion function.
Hence, deduce from the large argument asymptotic form of the plasma dispersion function that
in the limit
. Show that the approximate solution of the previous equation is
- Show that, when combined with the Maxwellian velocity distribution (8.24), the dispersion relation (8.49) reduces to
where
,
,
, and
is the plasma dispersion
function.
Use the large-argument expansion of the plasma dispersion function for the ions,
and the small-argument expansion for the electrons,
Substituting these expansions into the
dispersion relation, writing
, where
and
are both real,
and
, demonstrate that
and
- Derive Equation (8.74) from Equations (8.69) and (8.73).
- Derive Equation (8.82) from Equations (8.74) and (8.79).
- Derive Equations (8.89)-(8.91) from Equation (8.82).
- Derive Equations (8.94)-(8.96) from Equation (8.82).
- Derive Equations (8.102)-(8.105) from Equation (8.82).
- Derive Equation (8.119) from Equation (8.118).
- Derive Equation (8.120) from Equations (8.79) and (8.119).
- Derive Equation (8.124) from Equation (8.123).
- Demonstrate that the distribution function (8.131) possesses a minimum at
when
, but not otherwise.
- Verify formula (8.133).
- Consider an unmagnetized quasi-neutral plasma with stationary ions in which the electron velocity
distribution function takes the form
Demonstrate that the dispersion relation for electrostatic plasma waves can be written
where
. Assuming that
is real and positive, and that
lies in the upper half of the complex plane, show
that when the integrals are evaluated as contour integrals in the complex
-plane (closed in the lower half of the plane), making use of the residue theorem (Riley 1974), the previous dispersion relation reduces to
where
. Finally, in the small-
limit,
, demonstrate that the growth-rate of the most unstable mode
is
- Derive Equation (8.137) from Equations (8.134)-(8.136).
- Derive Equations (8.160) and (8.161) from Equations (8.154), (8.155), and (8.159).
Next: Bibliography
Up: Waves in Warm Plasmas
Previous: Harris Instability
Richard Fitzpatrick
2016-01-23