Generation of High-Power Sub-THz Waves in Magnetized Turbulent Electron Beam Plasmas
Sub-THz radiation can be generated by conversion of plasma waves into electromagnetic (EM) radiation in a plasma with strong Langmuir (LT) turbulence produced via a two-stream instability of a high current relativistic electron beam (REB). Nonlinear plasmon-plasmon merging results in the generation...
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Published in: | Journal of infrared, millimeter and terahertz waves Vol. 35; no. 1; pp. 81 - 90 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , |
Format: | Journal Article |
Language: | English |
Published: |
Boston
Springer US
2014
|
Subjects: | |
Online Access: | Get full text |
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Summary: | Sub-THz radiation can be generated by conversion of plasma waves into electromagnetic (EM) radiation in a plasma with strong Langmuir (LT) turbulence produced via a two-stream instability of a high current relativistic electron beam (REB). Nonlinear plasmon-plasmon merging results in the generation of photons nearby the 2
nd
harmonic of the plasma frequency 2
ω
p
(“2
ω
p
-process”). For plasma densities of 10
14
− 10
15
cm
−3
, these frequencies are in the range of sub-THz waves at 370–570 GHz. The specific power density of sub-THz-wave emission from plasmas in the multi-mirror magnetic trap GOL-3 (at BINP) during injection of a 10-μs-REB with a current density of about 1 kA/cm
2
at plasma densities
n
e
≈ 5∙10
14
cm
−3
, electron temperatures
T
e
≈ 1.5 keV and magnetic induction
B
≈ 4 T was measured to be approx. 1 kW/cm
3
in the frequency band around 300 GHz. In the case of a weakly relativistic 100-μs-electron beam (90 keV) with 250 A/cm
2
the corresponding results are 700 W/cm
3
around 90 GHz with an efficiency of 1–2 % at
n
e
≈ 3∙10
13
cm
−3
(total power ≈ 30 kW). Theoretical investigations show that at a density of
n
e
≈ 3∙10
15
cm
−3
and a turbulence level of 5 % the generated sub-THz power can reach ≈ 1 MW/cm
3
. |
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Bibliography: | ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
ISSN: | 1866-6892 1866-6906 |
DOI: | 10.1007/s10762-013-9969-3 |