Table 3-1 TM Scale Factor By UTM Easting
3-7 Gauss-Kruger Projection
a. General. The Gauss-Kruger Projection can be
described as the Transverse Mercator Projection
derived by mapping directly from an ellipsoid which is
tangent to the cylinder. See Figure 3-8. It is a
conformal projection with many similarities to the
Transverse Mercator Projection. The tangent point is
the meridian of longitude chosen as the Central
Meridian for the projection. As with Transverse
Mercator, the Gauss-Kruger Projection depicts 60
zones and area distortion is the same as described in
paragraph 3-6b above. Many geodesists consider the
Gauss-Kruger and Transverse Mercator Projections to
be the same, except for scale factor.
Figure 3-8 Gauss-Kruger Projection
b. Distortion of Lines. When a meridian is tangent to
a cylinder of projection, there is no distortion along
that line. Figure 3-9 shows that all lines which are not
located on the central meridian are longer on the
projected surface than they are on the ellipsoid. For
example, line A'M is longer than line AM when A
represents the meridian located three degrees from the
central meridian, A' is the projection of that meridian
onto a cylinder, and M is the central meridian (tangent
point).
c. Scale Factor. For the Gauss-Kruger Projection, the
scale factor at the central meridian is Unity (1.000 or
Exact). The factor increases outward toward the zone
limits in excess of 1.004 at the equator.
3-8 Polar Stereographic Projection
a. General. The Polar Stereographic Projection is
used for mapping the earth's polar regions and
identifies those regions as North and South zones. The
North zone extends from the North Pole to 83° 30' N
latitude; the South zone extends from the South Pole to
79° 30' S latitude. It is a conformal azimuthal
projection which is developed by projecting a polar
region onto a plane which is either tangent to an
ellipsoid at the pole or secant to the ellipsoid at a
specific latitude. This text will discuss only the secant
condition. See Figure 3-10. The plane is
perpendicular to the polar axis of the ellipsoid and the
origin of the projection is the opposite pole. See Figure
DRAFT
3-7