Abel inversion of a holographic interferogram for determination of the density profile of a sheared-flow Z pinch
Creators
- 1. Aerospace and Energetics Research Program, University of Washington, Seattle, Washington 98195-2250 (United States)
Description
A holographic interferometer is used to determine the radial electron number density profile of a sheared-flow Z pinch. Chord-integrated density information is recorded during a plasma pulse using the expanded beam of a pulsed ruby laser and holographic techniques. An Interactive Data Language (IDL) computer routine that requires only minimal user interaction is used to measure the resulting fringe shift in the reconstructed interferogram. This chord-integrated density information is inverted using an Abel inversion to determine the radial electron density profile. The density profiles obtained show a radially symmetric plasma column with an electron density of 1016-1017 cm-3 above the background plasma density. Holographic measurements are made at different times on separate plasma pulses to track the evolution of the density profile over time. These measurements are corroborated by time-dependent measurements made using a He-Ne interferometer
Additional details
Identifiers
- DOI
- 10.1063/1.2336082;
Publishing Information
- Journal Title
- Review of Scientific Instruments
- Journal Volume
- 77
- Journal Issue
- 8
- Journal Page Range
- p. 083502-083502.10
- ISSN
- 0034-6748
- CODEN
- RSINAK
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38026495
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- DENSITY; ELECTRON DENSITY; ELECTRONS; INTERFEROMETERS; INTERFEROMETRY; LIGHT TRANSMISSION; PLASMA; PLASMA DENSITY; PULSES; RUBY LASERS; SHEAR
- Descriptors DEC
- ELEMENTARY PARTICLES; FERMIONS; LASERS; LEPTONS; MEASURING INSTRUMENTS; PHYSICAL PROPERTIES; SOLID STATE LASERS; TRANSMISSION
Optional Information
- Notes
- (c) 2006 American Institute of Physics