Time-resolved measurements on reflectivity of an ultrafast laser-induced plasma mirror
Creators
- 1. State Key Laboratory of High Field Laser Physics, Shanghai Institute of Optics and Fine Mechanics, Chinese Academy of Sciences, P. O. Box 800-211, Shanghai 201800 (China)
Description
Using a linearly chirped laser pulse to irradiate antireflection coated targets, the time-varying reflectivity of a plasma mirror (PM) has been measured at various laser intensities from 1012 to 1017 W/cm2. The onset of plasma generation as well as the formation process of a PM with the highest reflectivity has been observed. The rise time of the PM's reflectivity reaching up to the maximum varies from 300-500 fs at lower laser intensities but goes up to 900 fs at higher intensity of >1016 W/cm2. This long rise time can be attributed to a slowly rising shoulder of the laser pulse, which will trigger the generation of preplasma well in advance of the laser peak. The detailed measurements on both time-integrated and time-resolved reflectivity of a PM, which is induced by p- and s-polarized laser pulses, respectively, indicate that an s-polarized pulse is favorable to obtain the maximal reflectivity and the best contrast improvement as well. This difference can be attributed to the weaker absorption and a smaller plasma scale length generated for s-polarization.
Additional details
Identifiers
- DOI
- 10.1063/1.3247865;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 16
- Journal Issue
- 10
- Journal Page Range
- p. 103104-103104.6
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41021652
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- LASER-PRODUCED PLASMA; MIRRORS; PULSE RISE TIME; REFLECTIVITY; TIME RESOLUTION
- Descriptors DEC
- OPTICAL PROPERTIES; PHYSICAL PROPERTIES; PLASMA; RESOLUTION; SURFACE PROPERTIES; TIMING PROPERTIES
Optional Information
- Notes
- (c) 2009 American Institute of Physics