Примери за използване на Main mirror на Английски и техните преводи на Български
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So here we have the main mirror.
Main mirror, heated, electrically adjustable.
To get rid of a duplicate of the main mirror in.
How to find out the main mirror of the site and configure it using a redirect.
For getting rid of a duplicate of the main mirror.
Firstly, the site contains a duplicate of the main mirror, the site opens with www and without it.
More than 100 air jets are also positioned behind the main mirror.
First, on the website has a duplicate of the main mirror, the site opens with www without him.
The humanitarian aura of the nation,or The defect of the main mirror.
There is a central hole in the main mirror through which the light passes and is brought to a focus by an eyepiece lens.
The focal length depends on the radius of the curve of the main mirror(lens).
The main mirror of the Newtonian reflector can be parabolic or even spherical if its aperture ratio is relatively small.
In 1993 NASA launched a mission to correct an issue with the telescope's main mirror.
The diameter of its main mirror is four times larger than any previous infrared space telescope and one and a half times larger than Hubble.
The first images sent back by the telescope were fuzzy because the telescope's main mirror was too flat.
Thediameter of Herschel's main mirror is four times larger than any other infraredspace telescope and 1.5 times larger than the Hubble Space Telescope.
Reflection of light rays from its surface converge to the ellipsoid's second focus which is behind the main mirror.
Focal length- this is the distance from the main mirror or the lens to the point where the light coming from the night objects is gathered.
Homemade telescope Many amateur astronomers prefer to collecttelescopes alone,buying only the most important elements- in particular, the main mirror.
Aperture- this is the diameter of the lens(with refractor telescopes),or the diameter of the main mirror(with reflector telescopes) and it is the most important characteristic of the telescopes.
One of the first reflectors was the Gregorian reflector telescope(1663), named after James Gregory,who invented a telescope with a parabolic main mirror.
It consist of four telescopes with main mirrors of 8.2m diameter, which are generally used separately but can be used together to achieve very high angular resolution.
The value of this parameter, measured in angular seconds,can be calculated when we divide the number 140 by the diameter of the main mirror(measured in millimeters).
The key feature and capabilities of the new ELT telescope will be in its main mirror, which will be composed of 798 hexagonal parts, the diameter of each of which will be 1.4 meters.
This huge telescope- its main mirror would be more than 100 metres across- would have a predicted resolution 40 times better than the Hubble Space Telescope and a sensitivity several thousand times greater.
It consists of four unit telescopes with main mirrors that are 8.2 meters(27 feet) in diameter; these telescopes are generally used separately but can also work together to achieve very high angular resolution.
The light, collected by a large main mirror, is reflected from a small elliptical mirror fixed in front of the main one and is led out to the observer through a hole in the center of the main mirror. .
Process technique for the main body: Mirror Polished.
For the main glaze on the mirror cake.