Diffraction of the Optical Wave in the Schmidt Cassegrain Telescope

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216305%3A26220%2F17%3APU123733" target="_blank" >RIV/00216305:26220/17:PU123733 - isvavai.cz</a>

Výsledek na webu

<a href="http://dx.doi.org/10.1109/COMITE.2017.7932303" target="_blank" >http://dx.doi.org/10.1109/COMITE.2017.7932303</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1109/COMITE.2017.7932303" target="_blank" >10.1109/COMITE.2017.7932303</a>

Jazyk výsledku

angličtina

Název v původním jazyce

Diffraction of the Optical Wave in the Schmidt Cassegrain Telescope

Popis výsledku v původním jazyce

The paper is focused on analysing of the distribution of optical intensity within a laser beam at the focal plane of the receiving optics which is affected mainly by diffraction of the optical wave in the Schmidt-Cassegrain telescope. The paper discusses the differences between diffraction of the optical wave on circular and annular aperture. In order to simplify the model of diffraction the Schmidt-Cassegrain telescope was approximated by annular aperture. This simplification seems to be valid according to experimental measurement which was carried out at the laboratory. The aim of the paper is to determine how the obscuration of the telescope affect the coupling efficiency of the Fully Photonic Receiver. Fully Photonic Receiver is used for direct coupling of the optical wave from free space to the single-mode optical fiber.

Název v anglickém jazyce

Diffraction of the Optical Wave in the Schmidt Cassegrain Telescope

Popis výsledku anglicky

The paper is focused on analysing of the distribution of optical intensity within a laser beam at the focal plane of the receiving optics which is affected mainly by diffraction of the optical wave in the Schmidt-Cassegrain telescope. The paper discusses the differences between diffraction of the optical wave on circular and annular aperture. In order to simplify the model of diffraction the Schmidt-Cassegrain telescope was approximated by annular aperture. This simplification seems to be valid according to experimental measurement which was carried out at the laboratory. The aim of the paper is to determine how the obscuration of the telescope affect the coupling efficiency of the Fully Photonic Receiver. Fully Photonic Receiver is used for direct coupling of the optical wave from free space to the single-mode optical fiber.

Druh

D - Stať ve sborníku

CEP obor

—

OECD FORD obor

20201 - Electrical and electronic engineering

Projekt

Výsledek vznikl pri realizaci vícero projektů. Více informací v záložce Projekty.

Návaznosti

P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Rok uplatnění

2017

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název statě ve sborníku

Microwave Techniques (COMITE), 2017 Conference on

ISBN

978-1-5090-4594-5

ISSN

—

e-ISSN

—

Počet stran výsledku

5

Strana od-do

1-5

Název nakladatele

IEEE

Místo vydání

Brno, Czech Republic

Místo konání akce

Brno

Datum konání akce

19. 4. 2017

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

000403400000006