Abstract
Conversion of dispersive longitudinal oscillation into electromagnetic radiation field in a non uniform warm fluid plasma is studied with the help of the linear equations of coupled wave fields deduced earlier by Chakraborty (1971). Expression for the radiated Poynting flux is obtained in the far field approximation.
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Abbreviations
- K 2t c 2 :
-
w 2−w 2e
- K 2e v 2e :
-
w 2−w 2e
- K 2i v 2i :
-
w 2−w 2i
- H :
-
magnetic field
- K :
-
wave vector
- K t :
-
wave vector of the transverse wave
- K e :
-
wave vector of the longitudinal wave in the electron fluid
- K i :
-
wave vector of the longitudinal wave in the ion fluid
- m :
-
electronic mass
- M :
-
ionic mass
- N 0 :
-
the number density of electrons an ions in the unpertubed state
- P e :
-
perturbation in the electron partial pressure
- Pi:
-
perturbation in the ion partial pressure
- N e :
-
perturbation in the electron number density
- N i :
-
perturbation in the ion number density
- v e :
-
the speed of sound in the electron fluid
- v i :
-
the speed of sound in the ion fluid
- w :
-
wave frequency
- μ 1 :
-
reduced mass
- K 1 :
-
wave vector of P
- N 1 :
-
uniform number density of electrons in the distant radiation field zone at the observation point
- P :
-
the perturbation in electron fluid pressure
- P 0 :
-
the amplitude of P
- r :
-
position vector
- r′ :
-
position vector in the scattering volume
- v :
-
scattering volume
- a :
-
distance of the order of molecular distances
- h :
-
extinction coefficient
- K 2l v 2e :
-
w 2−w 2e
- K 2t c 2 :
-
w 2−w 21
- r′ 1,2 :
-
integration points in V for evaluating E and H
- e 1, 2, 3 :
-
three mutually perpendicular unit vectors such that e 1 is parallel to grad N 0, e 2 in the plane containing e 1 and K 1 and e 3=[e 1×e 2]
- S t :
-
Poynting flux
- S l :
-
energy flux carried by the perturbations in density and pressure
- 〈S t〉:
-
average of S t over the time period 2π/w
- 〈S l〉:
-
average of S l over the time period 2π/w
- V 1 :
-
integration volume for the E field
- V 2 :
-
integration volume for the H field
- λ :
-
wave length of the radiation field
- θ :
-
angle between K t and grad N 0
- θ 0 :
-
angle between K 1 and grad N 0
- θ 1,2 :
-
K 0·r′ 1,2
- μ 0 :
-
|〈S t〉| cos θ/|〈S l〉| cos θ 0
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Visiting Fellow. Permanent Address: Mathematics Department, Jadavpur University, Calcutta-32, India.
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Chakraborty, B. Conversion of longitudinal waves into electromagnetic radiation by a non-uniform plasma. Appl. Sci. Res. 28, 466–476 (1973). https://doi.org/10.1007/BF00413084
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DOI: https://doi.org/10.1007/BF00413084