Published June 2005
| Version v1
Journal article
Temperature and melting of laser-shocked iron releasing into an LiF window
Creators
- 1. Dipartimento di Fisica, Universita degli Studi di Milano, Bicocca and INFM, piazza della Scienza 3, 20126 Milan (Italy)
- 2. Laboratoire pour l'Utilisation des Lasers Intenses (LULI), Ecole Polytechnique, 91128 Palaiseau (France)
Description
Absolute reflectivity and self-emission diagnostics are used to determine the gray-body equivalent temperature of laser-shocked iron partially releasing into a lithium fluoride window. Pressure and reflectivity are measured simultaneously by means of velocity interferometer system for any reflector interferometers. In the temperature-pressure plane, a temperature plateau in the release is observed which is attributed to iron's melting line. Extrapolation of data leads to a melting temperature at Earth's inner-outer core boundary of 7800±1200 K, in good agreement with previous works based on dynamic compression. Shock temperatures were calculated and found to be in the liquid phase
Additional details
Identifiers
- DOI
- 10.1063/1.1896375;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 12
- Journal Issue
- 6
- Journal Page Range
- p. 060701-060701.4
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37070313
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY; S36: MATERIALS SCIENCE;
- Descriptors DEI
- EXTRAPOLATION; INTERFEROMETRY; IRON; LASER RADIATION; LITHIUM FLUORIDES; MELTING POINTS; REFLECTIVITY; SHOCK WAVES
- Descriptors DEC
- ALKALI METAL COMPOUNDS; ELECTROMAGNETIC RADIATION; ELEMENTS; FLUORIDES; FLUORINE COMPOUNDS; HALIDES; HALOGEN COMPOUNDS; LITHIUM COMPOUNDS; LITHIUM HALIDES; MATHEMATICAL SOLUTIONS; METALS; NUMERICAL SOLUTION; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; RADIATIONS; SURFACE PROPERTIES; THERMODYNAMIC PROPERTIES; TRANSITION ELEMENTS; TRANSITION TEMPERATURE
Optional Information
- Notes
- (c) 2005 American Institute of Physics