Paper
28 September 2009 Simulations of ASE and seeded transient x-ray lasers using the COLAX code
Annie Klisnick, Olivier Larroche, François de Dortan, Jamil Habib, Olivier Guilbaud
Author Affiliations +
Abstract
We present recent calculations performed with the Maxwell-Bloch COLAX code. We investigate several features of transient X-ray lasers pumped with grazing incidence geometry and operated either with or without seeding by a highorder harmonics pulse. We show that the spontaneous emission source term included in the code accounts well for the speckle patterns observed in near-field and far-field images of the amplification of spontaneous emission (ASE) beams. Our calculations confirm the predictions of a simpler model based on the properties of spatial and temporal coherence of the source. We study the role of varying the level of the harmonic pulse seeded in the X-ray laser plasma. We show that the amplification factor and the contrast with respect to the ASE background cannot be maximized simultaneously. Finally we describe a recent upgrade of the code in which a time-dependent description of the populations of the lasing states has been implemented. This more rigorous treatment allows us to investigate the small-scale temporal behaviour of seeded X-ray lasers. The new version of the COLAX code was recently tested and preliminary results will be presented.
© (2009) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Annie Klisnick, Olivier Larroche, François de Dortan, Jamil Habib, and Olivier Guilbaud "Simulations of ASE and seeded transient x-ray lasers using the COLAX code", Proc. SPIE 7451, Soft X-Ray Lasers and Applications VIII, 74510U (28 September 2009); https://doi.org/10.1117/12.825511
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
X-ray lasers

Plasma

Picosecond phenomena

Near field

Data modeling

Optical simulations

Spatial coherence

Back to Top