Product Code Database
Example Keywords: sweater -stocking $73
   » » Wiki: Lensmeter
Tag Wiki 'Lensmeter'.
Tag

Lensmeter
 (

 C O N T E N T S 

[[Image:Lensmeter-2.png|thumb|300px|right| A simple lensmeter cross sectional view.

1 – Adjustable eyepiece 2 – Reticle
3 – Objective lens 4 – Keplerian telescope
5 – Lens holder 6 – Unknown lens
7 – Standard lens 8 – Illuminated target
9 – Light source 10 – Collimator
11 – Angle adjustment lever
12 – Power drum (+20 and -20 Diopters)
13 – Prism scale knob]]

A lensmeter or lensometer (sometimes even known as focimeter or vertometer), is an optical instrument used in . It is mainly used by and to measure the back or front vertex power of a spectacle lens and verify the correct prescription in a pair of , to properly orient and mark uncut lenses, and to confirm the correct mounting of lenses in spectacle frames. Lensmeters can also verify the power of , if a special lens support is used.

The parameters appraised by a lensmeter are the values specified by an or on the patient's prescription: sphere, cylinder, axis, add, and in some cases, prism. The lensmeter is also used to check the accuracy of , and is often capable of marking the lens center and various other measurements critical to proper performance of the lens. It may also be used prior to an to obtain the last prescription the patient was given, in order to expedite the subsequent examination.


History
In 1848, produced the photographometer, an instrument designed to measure the intensity of photogenic rays; and in 1849 he brought out the focimeter, for securing a perfect focus in photographic portraiture. In 1876, introduced a phakometer which was a similar set up to an which could measure the power and find the of a convex lens. Troppman went a step further in 1912, introducing the first direct measuring instrument.

In 1922, a patent was filed for the first projection lensmeter, which has a similar system to the standard lensmeter pictured above, but projects the measuring target onto a screen eliminating the need for correction of the observer's in the instrument itself and reducing the requirement to peer down a small telescope into the instrument. Despite these advantages the above design is still predominant in the optical world. accessed 20 Jan 2009


See also


External links

Page 1 of 1
1
Page 1 of 1
1

Account

Social:
Pages:  ..   .. 
Items:  .. 

Navigation

General: Atom Feed Atom Feed  .. 
Help:  ..   .. 
Category:  ..   .. 
Media:  ..   .. 
Posts:  ..   ..   .. 

Statistics

Page:  .. 
Summary:  .. 
1 Tags
10/10 Page Rank
5 Page Refs