Homework 1 Solution
GIS in Water Resources
Fall 2010
Prepared by David R. Maidment
1.
�Map Projection Parameters
The map below shows Utah and the display
parameters of the State Plane coordinate system for the Utah Central Zone.��
���������
(a)� Sketch on the map the standard parallels, the
central meridian and the latitude of origin of this projection.
I prepared the map above using ArcGIS Explorer Online.� http://explorer.arcgis.com/� The tool for
locating coordinates is called Measure �and when you click on that tool, it invokes a
dialog box
�within which the
�icon serves to select identifying a point
location.��� Utah is clearly defined in
latitude-longitude coordinates using meridians at 109�W and 114�W and parallels
at 37�N and 42�N, making it 5� longitude x 5� latitude in area, except for a
box 2� longitude x 1� latitude that is omitted in the upper right corner (I
imagine the reason for this would make an interesting historical study!)
(b)� For this projection, what are the coordinates
of the origin (fo, lo) and the corresponding (Xo, Yo) ?
(fo,
lo)
= (38� 20� N, 111� 30� W)
(Xo, Yo) = (1640416.666667, 6561666.666667) in meters.
Notice that the (fo, lo) are stated with the vertical coordinate first and the horizontal coordinate second, while the reverse is true for (Xo, Yo)
(c)� What earth datum is used in this coordinate
system?
The earth datum is GCS (Geographic Coordinate System) North American of 1983, or NAD83.
(d)�� What map projection is used in this
coordinate system?
Lambert Conformal
Conic
2. Locations on the Earth�
Using ArcGIS Explorer and putting in the names of Austin, Logan and Lincoln reveals the following designated locations for these cities.�� Convert these locations into decimal degrees.
The computations are shown in the spreadsheet below.�
LatDD = LatDeg + LatMin/60 + LatSec/3600
LongDD = -(LongDeg + LongMin/60 + LongSec/3600)
So, for Austin,
LatDD = 30 + 16/60 + 4/3600 = 30.2678
LongDD = -(97+44/60 + 35/3600) = -97.7431
LatDeg |
LatMin |
LatSec |
LongDeg |
LongMin |
LongSec |
LatDD |
LongDD |
|
Austin |
30 |
16 |
4 |
97 |
44 |
35 |
30.2678 |
-97.7431 |
Logan |
41 |
44 |
11 |
111 |
50 |
6 |
41.7364 |
-111.8350 |
Lincoln |
40 |
48 |
52 |
96 |
42 |
28 |
40.8144 |
-96.7078 |
The smallest unit that distinguishes location in degrees, minutes and seconds is 1 arc second.� This corresponds to 1/3600 = 0.000278 decimal degrees.� It follows that locations in decimal degrees must be specified to at least 4 decimal places if location precision is not to be lost when conversions into decimal degrees are done.� �Also, please note that in the western hemisphere, decimal longitudes are always negative.� In other word decimal degrees are positive or negative numbers not numbers with W or N associated with them.
3.� Great Circle Distances�
The great circle distance is given
by the formula
with R = 6378.137 km.
All the angles need to be in radians for formulas in Excel to work, so the above angles are converted as shown below:
|
LatDD |
LongDD |
LatRad |
LongRad |
||
Austin |
30.2678 |
-97.7431 |
0.528272 |
-1.70594 |
||
Logan |
41.7364 |
-111.8350 |
0.728437 |
-1.95189 |
||
Lincoln |
40.8144 |
-96.7078 |
0.712346 |
-1.68787 |
||
|
||||||
And the corresponding great earth distances are computed as follows:
R = |
6378.137 |
|||
Austin-Logan |
LatRad, f |
LongRad, l |
Distance km |
|
A |
0.5283 |
-1.7059 |
1795.473 |
|
B |
0.7284 |
-1.9519 |
||
Austin-Lincoln |
LatRad, f |
LongRad, l |
Distance km |
|
A |
0.5283 |
-1.7059 |
1177.762 |
|
B |
0.7123 |
-1.6879 |
||
Logan-Lincoln |
LatRad, f |
LongRad, l |
Distance km |
|
A |
0.7284 |
-1.9519 |
1268.081 |
|
B |
0.7123 |
-1.6879 |
In order to check the distances between the two points, I used ArcGIS Explorer at http://explorer.arcgis.com .� I marked the three cities as described above, and then I used a measure tool to measure between pairs of marked locations.�� Here is an example for the distance between Logan and Lincoln, for which I got 1267.787 km, as compared to 1268.081 km above (a difference of 0.294 km, or 294 m), which seems reasonable given that the great circle distance we�ve computed is on a spherical earth.
The distance between Austin and Logan is 1795.183 km, and between Austin and Lincoln is 1178.257 km which are both very close to the answers given above.� Actually, it�s a bit hard to zoom into these points exactly in ArcGIS Explorer when doing this �measure� so if you could do that better, the results would probably be closer to those computed by the great circle formula.�
4.� Size of DEM cells
The distances AB and AC, and be computed by the formulas for
distance along a parallel and a meridian, with Re = 1378.137 km.��
There is a very slight difference in the latitude f between the top and bottom of a DEM cell, but let�s neglect that for this example, so , the area of the DEM cell is given by
The results of a spreadsheet computation of these formulas are shown below:
DEM Cells |
R = |
6378.137 |
Df, Dl = |
4.848E-06 |
LatRad, f |
LongRad, l |
Cosf |
AB |
AC |
Area |
Sqrt(Area) |
|
Austin |
0.5283 |
-1.7059 |
0.8637 |
26.707 |
30.922 |
825.828 |
28.737 |
Logan |
0.7284 |
-1.9519 |
0.7462 |
23.075 |
30.922 |
713.513 |
26.712 |
Lincoln |
0.7123 |
-1.6879 |
0.7568 |
23.403 |
30.922 |
723.662 |
26.901 |
The great circle formula given above is erroneous when applied to very short distances.� In that case, an alternative great circle formula called the �Haversine formula� can be used, as follows:
In this case, for the distance along a parallel can
be given by the latitude of the location.��
Doing the calculations this way gives the following results, which are
identical to the ones given above for the simple formulas for distance along a
meridian and parallel.
DEM Cells |
R = |
6378.137 |
Df, Dl = |
4.848E-06 |
|||
LatRad, f |
LongRad, l |
Cosf |
AB |
AC |
Area |
Sqrt(Area) |
|
Austin |
0.528272 |
-1.7059381 |
0.8636792 |
26.707 |
30.922 |
825.828 |
28.737 |
Logan |
0.728437 |
-1.951889 |
0.7462155 |
23.075 |
30.922 |
713.513 |
26.712 |
Lincoln |
0.712346 |
-1.6878691 |
0.7568303 |
23.403 |
30.922 |
723.662 |
26.901 |
The fact that these two results are identical can also be demonstrated mathematically.
�For distance along a
parallel, �and in this case the Haversine
formula reduces to
as was given earlier in the simple formula for distance along a parallel.
�For distance along a
meridian, �so the Haversine
formula reduces to:
as was given earlier in the simple formula for distance along a meridian.�