Voorbeelden van het gebruik van Primary mirror in het Engels en hun vertalingen in het Nederlands
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Colloquial
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Official
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Ecclesiastic
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Medicine
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Financial
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Computer
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Ecclesiastic
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Official/political
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Programming
The primary mirror is what we're looking at right now.
Artists's Rendering of the primary mirror of the ELT.
The telescope's primary mirror rests on a support structure that was designed in the Netherlands.
Optical telescopes collect light from the cosmos using a primary mirror.
The primary mirror consists of 798 segments,
The Large Binocular Telescope had its first light with a single primary mirror on October 12, 2005, which was a view of NGC 891.
The telescope's primary mirror will have a diameter of 6.5 m(260 in)
Like the Schmidt telescope, the Maksutov corrects for spherical aberration by placing a corrector lens in front of the primary mirror.
Its spherical primary mirror consists of 91 identical hexagonal segments, each one meter in size.
Analysis of the flawed images showed that the cause of the problem was that the primary mirror had been ground to the wrong shape.
The second primary mirror was installed in January 2006
The hexagonal, mechatronic supporting structure holds the primary mirror of the telescope in the desired shape with nanometre precision.
The second primary mirror was installed in January 2006
meet the challenges of the ELT, which will have a revolutionary 40-metre-class diameter primary mirror.
The primary mirror consists of 798 hexagonal mirror segments,
These coating operations are required by the harsh climate conditions such as sandstorms that are liable to affect the silver layers of the primary mirror.
This Newtonian, with a 6-inch-diameter(150 mm) primary mirror, compared favorably with the large aerial refracting telescopes of the day.
we are really referring to the diameter of its primary mirror.
The VST comprises two mirrors, a primary mirror(M1) with a diameter of 2.61 m
saw first light with a single primary mirror on October 12, 2005 which viewed NGC 891.
The VST comprises two mirrors, a primary mirror(M1) with a diameter of 2.61 m
related auxiliary equipment for the Primary Mirror have been contracted to the VDL Groep.
Its primary mirror is 15 metres across:
All four instruments were mounted directly behind the primary mirror of the telescope, in a circular arrangement,
Bigger primary mirrors allow astronomers to capture more light
A pyramid-shaped mirror behind the primary mirror of the telescope distributed the infrared light to the four instruments,