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lines  in  the  map.  For  example,  it  may  be  constant  along  any  given
                                                                                           th
                  parallel. This would mean that features lying on the 20  parallel are
                                                                   th
                  equally  distorted,  features  on  the  40   parallel  are  equally  distorted
                                                                 th
                  (but differently from those on the 20  parallel), and so on.
                        2. Area. If a map preserves area, then the size of a feature on a
                  map is the same relative to its size on the earth. For example, on an
                  equal-area world map, Norway takes up the same percentage of map

                  space that actual Norway takes up on the earth. To look at it another
                  way, a coin moved to different spots on the map represents the same
                  amount of actual ground no matter where you put it. In an equal-area
                  map, the shapes of most features are distorted. No map can preserve

                  both shape and area for the whole world, although some come close
                  over sizeable regions.
                        3. Distance. If a line from a to b on a map is the same distance

                  (accounting for scale) that it is on the earth, then the map line has true
                  scale. No map has true scale everywhere, but most maps have at least
                  one  or  two  lines  of  true  scale.  An  equidistant  map  is  one  that

                  preserves  true  scale  for  all  straight  lines  passing  through  a  single,
                  specified  point.  For  example,  in  an  equidistant  map  centered  on
                  Redlands,  California,  a  linear  measurement  from  Redlands  to  any

                  other point on the map would be correct.
                        4. Direction or azimuth (figure 6.3.), is measured in degrees of
                  angle from north. On the earth, this means that the direction from a to
                  b  is  the  angle  between  the  meridian  on  which  a  lies  and  the  great

                  circle arc connecting a to b.
























                                 Figure 6.3. The azimuth of a to b is 22 degrees.



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