1. Proposal of new optic elements G. Chadzitaskos Department of Physics, FNSPE, Czech Technical University in Prague Stará Lesná 2012

2. Overview F Two diffraction grating F Parabolic strip telescope F Objective for X ray microscopy F CNOT on polarizated states of light F Objective for X ray telescope

3. Two diffraction systém (Wikipedia)

4. . Two diffraction system The light from monochromatic light source 1 is divided into two channels 3, by a 1:1 beam splitter 2, and is brought into the two- diffraction gratings 5. Two-diffraction grating generally consists of a large number of equally spaced slits, which allows connection of one channel with odd slits and the other channel with even slits 4. Then spots 7 – interference maxima – appear on the screen 6.

5. Maxima case 1 : case 2:

6. Intensities

7. Exploitation Measurement of coincident part of light Measurement of cross sections of interaction light and electrons (two slit experiment)

8. CNOT ON POLARIZATED STATES OF COHERENT LIGHT Optical activity of molecules with magnetic dipole

9. (C.Denz,Electro-optic composite polymers, Munster)

10. Linear dependence on electric field

11. Exploitation Quantum optics

12. PARABOLIC STRIP TELESCOPE Principle Rotation around y axis and Radon inverse transform

13. Used experimental plexiglass telescope objectives

14. Artifitial constelations

15. Image procesing F From camera RGB uint8 F Select central part, make matrices 600 x 600x 3 and rotate, single precision F 12th root of real matrices F Point multiplication of 0 and 90 degree matrices F Point multiplication, optimalization F Uint8 and image

16. Images of artificial star constellation Original images at 0, 45, 90, and 135 degree After MATLAB calculation

17. Image procesing

18. Advantages \ good angular resolution low expenses simple technological development simple exploitation of adaptive optics possibility to install a net of large telescopes over the Earth lower weight for use on satellites Proposal: Over Earth net of telescopes (30 degrees) high mounting not necessary low wind influence low gravitational influence

19. Objective for X ray microscopy Fresnel zone plates, polycapillar optics, Goebel mirrors, biconcave refractive optics. New: Spatial grating – Bragg’s and interference conditions

20. . Example

22. X ray telescope Wolter Kirkpatrick-Baez Lobster eye objective

23. New X-ray telescope

24. Bragg’s condition

25. Děkuji za pozornost

26. F Pro destičku germaniového monokrystalu a teploty mezi 250 a 1000 K je pro vlnovou délku 0.5 nm hodnota například pro xmin = 10 cm bude xmax = 10,8 cm.