Angular distribution separation of the extreme ultraviolet emission and suprathermal ions with energy reduction

Author:

Niinuma Takeru1ORCID,Sugiura Tsukasa1,Morita Hiroki1ORCID,Jiang Weihua2ORCID,Sakaue Kazuyuki3ORCID,O'Sullivan Gerry4ORCID,Namba Shinichi5ORCID,Higashiguchi Takeshi1ORCID

Affiliation:

1. Department of Electrical and Electronic Engineering, Faculty of Engineering, Utsunomiya University 1 , 7-1-2 Yoto, Utsunomiya, Tochigi 321-8585, Japan

2. Department of Electrical Engineering, Nagaoka University of Technology 2 , Nagaoka, Niigata 940-2188, Japan

3. Nuclear Professional School, School of Engineering, The University of Tokyo 3 , 7-3-1 Hongo, Bunkyo, Tokyo 113-8656, Japan

4. School of Physics, University College Dublin 4 , Belfield, Dublin 4, Ireland

5. Department of Advanced Science and Engineering, Hiroshima University 5 , 1-4-1 Kagamiyama, Higashihiroshima, Hiroshima 739-8527, Japan

Abstract

We have demonstrated angular distribution separation of the extreme ultraviolet (EUV) emission and suprathermal ions with a significant energy reduction for ions produced using dual pulse irradiation of a planar gadolinium (Gd) target. The pulse separation time between the pre-pulse and the main laser heating pulse was set at 30 ns, and the pre-plasma was irradiated at a distance of 50 μm above the target. Angular distributions of the EUV emission and the suprathermal ions were almost isotropic and followed a  cos4θ distribution, respectively. The suprathermal ions were emitted normal to the target along the pre-pulse laser axis. The most probable energy of the suprathermal ions was less than 2 keV, while their maximum charge state was Gd6+ with the pre-plasma, compared to an energy of about 10 keV with a maximum charge state Gd15+ without the pre-plasma. The results suggest that the collector mirror position may be chosen to achieve a long lifetime, by avoiding damage from fast ion collisions.

Funder

Japan Society for the Promotion of Science

Sumitomo Foundation

Publisher

AIP Publishing

Subject

Physics and Astronomy (miscellaneous)

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