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Magnification is the process of enlarging something only in appearance, not physical size. Magnification is also a number describing by which factor an object was magnified. In some fields, this number may be less than one, corresponding to an apparent reduction in size. This is sometimes called '''minification'''.

Typically magnification is related to scaling up Visual s or Images to be able to see more detail, increasing Resolution , using Optics , Printing techniques, or Digital Processing . In all cases, the magnification of the image does not change the Perspective of the image.


MAGNIFICATION AS A NUMBER (OPTICAL MAGNIFICATION)


Optical magnification is the ratio between the apparent size of an object (or its size in an image) and its true size, and thus it is a Dimensionless Number .

  • Linear magnification — For Real Image s, e.g., images projected on a screen, ''size'' means a linear dimension (measured, e.g., in millimeters or Inch es).


  • Angular magnification — For Optical Instrument s with an Eyepiece , the linear dimension of the image seen in the eyepiece ( Virtual Image in infinite distance) cannot be given, thus ''size'' means the angle subtended by the object at the focal point ( Angular Size ). Strictly speaking, one should take the Tangent of that angle (in practice, this makes a difference only if the angle is larger than a few degrees). Thus, angular magnification is defined as

    • ::\mathrm{MA}= rac{ an arepsilon}{ an arepsilon_0},

:where { arepsilon_0} is the angle subtended by the object at the front focal point of the objective and { arepsilon} is the angle subtended by the image at the rear focal point of the eyepiece.
  • Example: The Angular Size of the full moon is 0.5°, in Binoculars with 10x magnification it appears to subtend an angle of 5°, which is roughly 1/10th of the field of view of typical Eyepiece s.


:By convention, for Magnifying Glass es and optical Microscope s, where the size of the object is a linear dimension and the apparent size is an angle, the magnification is the ratio between the apparent (angular) size as seen in the eyepiece and the angular size of the object when placed at the conventional closest distance of distinct vision of 25 cm from the eye.

Optical magnification is sometimes referred to as "power" (e.g. "10x power"), although this can lead to confusion with Optical Power .


Calculating the magnification of optical systems


  • is

    • ::M = {f \over f-S}

:where ''f'' is the focal length and ''S'' is the distance from the lens to the object. Note that for Real Image s, ''M'' is negative and the image is inverted. For Virtual Image s, ''M'' is positive and the image is upright.
  • Telescope : The linear magnification is given by

    • ::M= {f_e \over f_o}

:where f_o is the Focal Length of the Objective Lens and f_e is the Focal Length of the Eyepiece . The angular magnification is given by
::\mathrm{MA}= {f_o \over f_e}
  • Magnifying Glass : The angular magnification of a magnifying glass depends on how the glass and the object are held, relative to the eye. If the lens is held such that its front focal point is on the object being viewed, the relaxed eye can view the image with angular magnification

    • ::\mathrm{MA}={25\ \mathrm{cm}\over f}\quad.

:If instead the lens is held very close to the eye, and the object is placed close to the lens, a larger angular magnification can be obtained, approaching
::\mathrm{MA}={25\ \mathrm{cm}\over f}+1\quad .
:Here, f is the Focal Length of the Lens in centimeters. The constant 25 cm is an estimate of the "near point" distance of the eye—the closest distance at which the eye can focus.
  • Microscope : The angular magnification is given by

    • ::\mathrm{MA}=M_o imes M_e

:where M_o is the magnification of the objective and M_e the magnification of the eyepiece. The magnification of the objective depends on its Focal Length f_o and on the distance d between objective back focal plane and the Focal Plane of the Eyepiece (called the tube length):
::M_o={d \over f_o}.
:The magnification of the eyepiece depends upon its focal length f_e and can be calculated by the same equation as that of a magnifying glass (above).

Note that both astronomical telescopes as well as simple microscopes produce an inverted image, thus the equation for the magnification of a telescope or microscope is often given with a Minus Sign .


Measurement of telescope magnification

Measuring the actual angular magnification of a telescope is difficult, but it is possible to use the reciprocal relationship between the linear magnification and the angular magnification, since the linear magnification is constant for all objects.

The telescope is focussed correctly for viewing objects at the distance for which the angular magnification is to be determined and then the object glass is used as an object the image of which is known as the Ramsden Disc . The diameter of this may be measured using an instrument known as a Ramsden Dynamometer which consists of a Ramsden eyepiece with micrometer cross hairs in the back focal plane. This is mounted in front of the telescope eyepiece and used to measure the diameter of the Ramsden disc. This will be much smaller than the object glass diameter, which gives the linear magnification (actually a reduction), the angular magnification can be determined from
:\mathrm{MA} =1 / M = D_{\mathrm{Objective}}/{D_\mathrm{Ramsden}}


OTHER USES


  • One can also ''magnify'' sounds (see Amplification ).

  • Magnification can also be used as a generalized term for increasing the detail or vividness of something: Ideas , Emotion s, etc.

  • A Magnification factor is sometimes misused on the internet to desribe the scale of an image e.g. from a microscopic. Magnification is not the correct term here because the size of the displayed image cannot be controlled. A better practice is to include a scale bar or other object of known size in the image. In certain art-pictures, such as Nikon Small World Gallery , scale bars are undesirable for aeshthetic reasons - in such cases, a caption is often used stating the size of some apparent feature or state the field size of the original image.



SEE ALSO