Issue |
J. Phys. Colloques
Volume 49, Number C1, Mars 1988
IAU Colloquium N° 102 on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas
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Page(s) | C1-231 - C1-234 | |
DOI | https://doi.org/10.1051/jphyscol:1988147 |
IAU Colloquium N° 102 on UV and X-ray Spectroscopy of Astrophysical and Laboratory Plasmas
J. Phys. Colloques 49 (1988) C1-231-C1-234
DOI: 10.1051/jphyscol:1988147
1 Astronomical Institute of the Czechoslovak Academy of Sciences, Ondejov, Czechoslovakia
2 Institute for Material Research, Praha, Czechoslovakia
3 Institute for Plasma Physics and Laser Microfusion, Warszawa, Poland
J. Phys. Colloques 49 (1988) C1-231-C1-234
DOI: 10.1051/jphyscol:1988147
THE POSSIBILITIES OF THE USE OF REPLICA X-RAY IMAGING MIRRORS IN PLASMA DIAGNOSTICS
R. HUDEC1, B. VALNÍCEK1, L. SVÁTEK2, V. LANDA2 et H. FIEDOROWICZ31 Astronomical Institute of the Czechoslovak Academy of Sciences, Ondejov, Czechoslovakia
2 Institute for Material Research, Praha, Czechoslovakia
3 Institute for Plasma Physics and Laser Microfusion, Warszawa, Poland
Abstract
The replica technology based on galvanoplastics offers the unique possibility of manufacturing of precise light-weight and low-cost imaging X-ray mirrors having both very small and large apertures of various types (paraboloid-hyperboloid, paraboloid-paraboloid, elipsoid-hyperboloid). Some of the further advantages such as the wide use of X-ray microscopic systems and the possibility to built large arrays of identical optical systems for simultaneous multispectral analysis are discussed together with the presentation of some examples of the manufactured mirrors. The first preliminary results are also presented.