The principle of the technology and design of the parabolic strip telescope

Kód výsledku v IS VaVaI

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Výsledek na webu

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DOI - Digital Object Identifier

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Jazyk výsledku

angličtina

Název v původním jazyce

The principle of the technology and design of the parabolic strip telescope

Popis výsledku v původním jazyce

Contribution of this paper is a proposal of the new special type of telescope with a parabolic strip as a primary element for astronomical observations or for measurements with good angular resolution in one direction. The observed objects are displayedas lines in the image plane of a length equal to the width of the mirror strip. If we observe a sufficiently bright object, the observation allows us to distinguish fine detail or fine movements on the sky. Each line segment corresponds to the integral intensity of the incident light from the observed object in the direction perpendicular to the mirror strip. For the reconstruction of the whole image with good resolution we need a parabolic mirror strip to rotate around the optical axis, and a series ofsequential snaps with a special camera. Different algorithms for reconstruction of the image are used. The main advantage of this rotating telescope is mechanical and manufacturing technological simplicity and an innovative design. Nothi

Název v anglickém jazyce

The principle of the technology and design of the parabolic strip telescope

Popis výsledku anglicky

Contribution of this paper is a proposal of the new special type of telescope with a parabolic strip as a primary element for astronomical observations or for measurements with good angular resolution in one direction. The observed objects are displayedas lines in the image plane of a length equal to the width of the mirror strip. If we observe a sufficiently bright object, the observation allows us to distinguish fine detail or fine movements on the sky. Each line segment corresponds to the integral intensity of the incident light from the observed object in the direction perpendicular to the mirror strip. For the reconstruction of the whole image with good resolution we need a parabolic mirror strip to rotate around the optical axis, and a series ofsequential snaps with a special camera. Different algorithms for reconstruction of the image are used. The main advantage of this rotating telescope is mechanical and manufacturing technological simplicity and an innovative design. Nothi

Druh

D - Stať ve sborníku

CEP obor

JR - Ostatní strojírenství

OECD FORD obor

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Projekt

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Návaznosti

S - Specificky vyzkum na vysokych skolach

Rok uplatnění

2014

Kód důvěrnosti údajů

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

Název statě ve sborníku

PIERS 2014 Guangzhou

ISBN

978-1-934142-28-8

ISSN

1559-9450

e-ISSN

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Počet stran výsledku

4

Strana od-do

1726-1729

Název nakladatele

Electromagnetics Academy

Místo vydání

Cambridge

Místo konání akce

Guangzhou

Datum konání akce

25. 8. 2014

Typ akce podle státní příslušnosti

WRD - Celosvětová akce

Kód UT WoS článku

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