- Derive the dispersion relation (7.28) from Equations (7.23)–(7.27).
- Show that the dispersion relation (7.28) can be written
where
,
,
,
, and
Demonstrate that, in the limit ,
, the approximate solution is
- Show that, when combined with the Maxwellian velocity distribution (7.24), the dispersion relation (7.23) 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 (7.24), the dispersion relation (7.49) 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 (7.74) from Equations (7.69) and (7.73).
- Derive Equation (7.82) from Equations (7.74) and (7.79).
- Derive Equations (7.89)–(7.91) from Equation (7.82).
- Derive Equations (7.94)–(7.96) from Equation (7.82).
- Derive Equations (7.102)–(7.105) from Equation (7.82).
- Derive Equation (7.119) from Equation (7.118).
- Derive Equation (7.120) from Equations (7.79) and (7.119).
- Derive Equation (7.124) from Equation (7.123).
- Demonstrate that the distribution function (7.131) possesses a minimum at when
, but not otherwise.
- Verify formula (7.133).
- 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 (7.137) from Equations (7.134)–(7.136).
- Derive Equations (7.160) and (7.161) from Equations (7.154), (7.155), and (7.159).