FREE BOOKS

Author's List




PREV.   NEXT  
|<   36   37   38   39   40   41   42   43   44   45   46   47   48   49   50   51   52   53   54   55   56   57   58   59   60  
61   62   63   64   65   66   67   68   69   70   71   72   73   74   75   76   77   78   79   80   81   82   83   84   85   >>   >|  
position of eyepiece when used the with the plane. When the plane is not in the way, the converging beam goes back to the eyepiece, _c_. When the plane, _d_, is introduced, the beam is turned at a right angle, and if it is a perfect surface, not only does the focal plane remain exactly of the same length, but the expanded star disks, are similar on either side of the focal plane. [Illustration: FIG. 9.] I might go on to elaborate this method, to show how it may be made still more exact, but as it will come under the discussion of spherical surfaces, I will leave it for the present. Unfortunately for this process, it demands a large truly spherical surface, which is just as difficult of attainment as any form of regular surface. We come now to an instrument that does not depend upon optical means for detecting errors of surface, namely, the spherometer, which as the name would indicate means sphere measure, but it is about as well adapted for plane as it is for spherical work, and Prof. Harkness has been, using one for some time past in determining the errors of the plane mirrors used in the transit of Venus photographic instruments. At the meeting of the American Association of Science in Philadelphia, there was quite a discussion as to the relative merits of the spherometer test and another form which I shall presently mention, Prof. Harkness claiming that he could, by the use of the spherometer, detect errors bordering closely on one five-hundred-thousandth of an inch. Some physicists express doubt on this, but Prof. Harkness has no doubt worked with very sensitive instruments, and over very small areas at one time. I have not had occasion to use this instrument in my own work, as a more simple, delicate, and efficient method was at my command, but for one measurement of convex surfaces I know of nothing that can take its place. I will briefly describe the method of using it. [Illustration: FIG. 10.] The usual form of the instrument is shown in Fig. 4; _a_ is a steel screw working in the nut of the stout tripod frame, _b_; _c c c_ are three legs with carefully prepared points; _d_ is a divided standard to read the whole number of revolutions of the screw, _a_, the edge of which also serves the purpose of a pointer to read off the division on the top of the milled head, _e_. Still further refinement may be had by placing a vernier here. To measure a plane or curved surface with this instrument, a perfect pla
PREV.   NEXT  
|<   36   37   38   39   40   41   42   43   44   45   46   47   48   49   50   51   52   53   54   55   56   57   58   59   60  
61   62   63   64   65   66   67   68   69   70   71   72   73   74   75   76   77   78   79   80   81   82   83   84   85   >>   >|  



Top keywords:

surface

 

instrument

 

spherometer

 

spherical

 

method

 
errors
 

Harkness

 

discussion

 

instruments

 

measure


surfaces
 

perfect

 

Illustration

 

eyepiece

 

efficient

 

command

 

measurement

 
convex
 

delicate

 

simple


briefly

 

describe

 

occasion

 

physicists

 

thousandth

 

hundred

 
closely
 
express
 

sensitive

 
worked

curved

 

serves

 

revolutions

 
number
 

standard

 

position

 

purpose

 

pointer

 
milled
 

division


divided

 

points

 

bordering

 

working

 

vernier

 

refinement

 
placing
 
carefully
 

prepared

 

tripod