Loading…
High sensitivity imaging Thomson scattering for low temperature plasma
A highly sensitive imaging Thomson scattering system was developed for low temperature ( 0.1 - 10 eV ) plasma applications at the Pilot-PSI linear plasma generator. The essential parts of the diagnostic are a neodymium doped yttrium aluminum garnet laser operating at the second harmonic ( 532 nm ) ,...
Saved in:
Published in: | Review of scientific instruments 2008-01, Vol.79 (1), p.013505-013505-8 |
---|---|
Main Authors: | , , , , , , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Summary: | A highly sensitive imaging Thomson scattering system was developed for low temperature
(
0.1
-
10
eV
)
plasma applications at the Pilot-PSI linear plasma generator. The essential parts of the diagnostic are a neodymium doped yttrium aluminum garnet laser operating at the second harmonic
(
532
nm
)
, a laser beam line with a unique stray light suppression system and a detection branch consisting of a Littrow spectrometer equipped with an efficient detector based on a "Generation III" image intensifier combined with an intensified charged coupled device camera. The system is capable of measuring electron density and temperature profiles of a plasma column of
30
mm
in diameter with a spatial resolution of
0.6
mm
and an observational error of 3% in the electron density
(
n
e
)
and 6% in the electron temperature
(
T
e
)
at
n
e
=
4
×
10
19
m
−
3
. This is achievable at an accumulated laser input energy of
11
J
(from 30 laser pulses at
10
Hz
repetition frequency). The stray light contribution is below
9
×
10
17
m
−
3
in electron density equivalents by the application of a unique stray light suppression system. The amount of laser energy that is required for a
n
e
and
T
e
measurement is
7
×
10
20
∕
n
e
J
, which means that single shot measurements are possible for
n
e
>
2
×
10
21
m
−
3
. |
---|---|
ISSN: | 0034-6748 1089-7623 |
DOI: | 10.1063/1.2832333 |