Page 25 - A Practical Introduction to Optical Mineralogy
P. 25

THE  MICROSCOPIC STUDY  OF MINERALS   THE  REFLECTED-LIGHT MICROSCOPE

 Zoning is generally a growth phenomenon and is therefore related to
 the crystal shape.
 Dispersion
 Refractive index increases as the wavelength oflight decreases. Thus the
 refractive index of a mineral for red light is less than for blue light (since
 the wavelength of red light is greater than the wavelength of blue light).
 White  light entering a  mineral  section  is  split  into  the  colours  of the
 spectrum, with blue nearest to the normal (i.e. the straight through path)
 and red the furthest away. This breaking up of the white light is called
 dispersion. In most minerals the amount of dispersion is very small and
 will  not  affect  the  mineral's optical  properties.  However, the Na-rich
                                            l~>,-----4- heat absorbing filter
 clinopyroxenes, the Na-rich amphiboles, sphene, chloritoid, zircon and   aperture diaphragm
 ?rookite possess very strong dispersion. With  many of these minerals,   Smith
       illuminator                                    field
 mterference figures  may be difficult to obtain and the use of accessory   .,__ ______ diaphragm
 plates (to determine  mineral  sign etc.)  may  not be possible.
                               l.~~:::l-..b;==------- focusing
        revolving                                     control
 Each mineral possesses a few  diagnostic properties, and in  the descrip-  objective
         changer
 tions in Chapter 2 these have been marked with an asterisk. Sometimes
 a  final  paragraph  discusses  differences  between  the  mineral  being   stage
         centring ------<1----1--"'""
 described and other minerals  that have similar optical  properties.   screws
          coarse
           focus
 1.4  The reflected-light microscope
 The light source   fine  focus
 A high intensity source (Fig.  1.3) is required for reflected-light studies,
 mainly  because  of  the  low  brightness  of  crossed  polar  images.
 Tungsten-halogen quartz lamps are  used, similar to those in  transpa-
 rency  projectors,  and the  tungsten  light  (A source)  gives  the  field  a
 yellowish tint. Many microscopists prefer to use a blue correction filter
 to change the light colour to that of daylight (C source). A  monochro-
 matic light source (coloured light corresponding to a very limited range
 of the  visible  spectrum)  is  rarely used  in  qualitative  microscopy, but
      Figure 1.3  The Vickers M73 reflected light microscope. Note that it is the polariser that rotates in
 monochromatic  filters  for  the  four  standard  wavelengths  ( 4 70 nm,
      !his microscope.
 546 nm,  589 nm  and  650 nm)  could  be  useful  in  comparing  the
 brightness  of  coexisting  minerals,  especially  now  that  quantitative
 measurements of brightness are readily available.
 The polariser    The incident illuminator
 Polarised light is  usually  obtained by  using  a polarising film,  and this   The incident illuminator sits above the objective and its  purpose is  to
 should be protected from the heat of the lamp by a glass heat filter. The   reflect light down through the objective on to the polished specimen. As
 polariser should always be inserted in the optical train. It is best fixed in   the reflected light travels back up through the objective to the eyepiece it
 orientation to give E-W vibrating incident light. However, it is useful to   must be possible for this light to pass through the incident illuminator.
 be able to rotate the polariser on occasion in order to correct its orien-  There  are  three  types  of  reflector  used  in  incident  illuminators
                   (Fig.  1.4):
 tation  or as  an alternative to rotating the analyser.
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