It does not. For an explanation of "focal plane" see the question
What is the focal plane?
The focal plane, or principal plane of focus, is the plane upon which the lens is actually focused. This distance is often represented on the lens barrel upon the distance scale. In a perfect lens, all of the light rays emanating from any point (meaning a "singularity", not a "place") that lies in that plane of space will converge in exactly the same place upon the film. ( . ) Any point before or beyond that plane will reproduce as a circle. ( o ) If the circle (known as a circle of confusion) is small enough, it is acceptably sharp to our eye, so it also appears to be in focus. This is what gives us 'depth of field', which is the distance before and after the focal plane that appears to be sharp. Of course, this perception depends mainly on the degree of magnification of the image. If these out-of-focus circles are enlarged enough, we can detect they are not actually points. The focal plane is not to be confused with the film plane.
A focal plane shutter is located right in front of the film or sensor where the light coming in from the lens is focused. Older film cameras would use an in-lens shutter system, sometimes even combined with the aperture mechanism. Focal plane shutters are used in modern cameras because they provide quicker shutter action and better camera balance.
The focal length of a camera's lens refers to the the magnification or telephoto power of the lens and is expressed in the millimeters of the lens, like 100mm, 300mm, etc. www.goldprints.com
When an earthquake is sourced, the coulomb stresses that originate from the source (due to the P-wave) are bounded by two perpendicular planes, which make up the 2 planes in an earthquake focal mechanism. Both are mathematically equivalent. Thus, without independent knowledge of which plane sourced the earthquake, either could be the "fault". Therefore, the axillary plane represents the mathematical equivalent to the source of the earthquake and is represented in earthquake focal mechanisms for a variety of reasons (helps visualize the style of faulting, disambiguity, completeness, etc.) It is extremely common for seismologists to calculate the focal mechanism without knowing which plane is the fault and which is the auxillary plane
The word magnification is a noun. It is the act of magnifying.
It does not. For an explanation of "focal plane" see the question What is the focal plane?
parafocal lenses are zoom lenses that preserve the focal plane for every magnification factor.
A plane mirror does not change the size of the (virtual) image reflected from it. Therefore, the magnification is 1.
The magnification of the telescope image is(focal length of the objective) divided by (focal length of the eyepiece).The focal length of the objective is fixed.Decreasing the focal length of the eyepiece increases the magnification of the image.(But it also makes the image dimmer.)
The magnification of a telescope M is the the focal length of the objective Fo over the focal length of the eyepiece Fe so increasing the focal length of the objective increases the magnification. The magnification of a microscope M is approximately tube length L/Fo x 25/Fe. Therefore increasing the focal length of the objective reduces the magnification.
The magnification of the telescope image is(focal length of the objective) divided by (focal length of the eyepiece).The focal length of the objective is fixed.Decreasing the focal length of the eyepiece increases the magnification of the image.(But it also makes the image dimmer.)
The focal length of a telescope is directly related to the magnification in that the longer the focal length, the more magnification you get from the telsceope. How the focal length of a telescope relates to the length of the telescope itself depends on the design of the telescope. In a refracting telescope, the focal length is approximately the length of the telescope. In a reflecting telescope, the focal length is roughly two time the length of the telescope.
Divide the focal length of the objective lens by the focal length of the eyepiece.
A telescope consists of two lenses. 1) The main lens which collects the light ( it is relatively bigger that eyepiece). 2) Eye piece , through which we see. Magnification of a telescope depends on the focal length of the eye piece and the main lens. Magnification = Focal length of the main lens / Focal length of the eyepiece . For example : If the focal length of the main lens is 12 units and the focal length of the eyepiece is 2 units , then the magnification will be 12/2 = 6.When the focal length of the main lens is constant , the focal length of the eyepiece is inversely proportional to the magnification.
20
1.82 meters
If the focal lengths of the objective and eyepiece are equal,then the magnification is ' 1 '.