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Azimuth Determination From Solar Observations

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Title: Azimuth Determination From Solar Observations


1
Azimuth Determination FromSolar Observations
  • ALAN M BERARDUCCI
  • National Geomagnetism Program - US Geological
    Survey
  • geomag.usgs.gov

2
Methods of Azimuth Determination
  • Solar or Star Observations
  • GPS
  • Gyro compass

3
Equipment for Solar Observations
  • Theodolite with
  • Solar Filter
  • Tripod or Pillar
  • Watch or Clock
  • Map or GPS

4
Gurley Transit
5
Solar Filter
6
Direct Azimuth determination
7
Indirect Azimuth Determination
8
Azimuth Monument
9
Preparation
  • Synchronize clock to UTC.
  • Obtain Lat and Long from GPS or Map.
  • Set theodolite on tripod or pillar.
  • Measurements made anytime except near noon.

10
Methodology
  • Horizontal angles for azimuth and sun.
  • Forward and reverse angles to Azimuth before and
    after sun readings.
  • Equal number of forward and reverse readings to
    sun.
  • Time accuracy to within 1 second.
  • 2 to 8 sun readings on sun per set.
  • 2 morning and 2 afternoon sets.

11
Sun in Crosshair - Zeiss
12
Sun in Crosshair Right or Left edge
13
Solar Observations Step 1-Sight the Azimuth Mark
  • Place the vertical circle on the right with the
    telescope aimed at the azimuth mark.
  • Precisely align the cross hairs with the azimuth
    mark.
  • Record the horizontal circle reading on the
    observation form.
  • Rotate the theodolite 180 so that the vertical
    circle is on the left with the telescope aimed at
    the azimuth mark.
  • Precisely align the cross lines with the azimuth
    mark.
  • Record the horizontal circle reading on the
    observation form.

14
Solar ObservationsStep 2 Find sun in the
telescope
  • Caution Never look at the sun through the
    telescope without a solar filter.
  • Orient the horizontal circle so the telescope is
    facing the sun. Tip the objective end of the
    scope downward so that a shadow from the sun
    shows on the base of the theodolite.
  • Do not look through the telescope during this
    procedure. Orient the shadow so that it is
    precisely centred on the theodolite base. Rotate
    the telescope upward until the bright light of
    the sun is visible through the telescope.
  • Place the solar filter on the telescope. Look
    through the telescope and focus the sun so the
    edges are well defined. The Zeiss Jena
    theodolite has a circular hair which is a bit
    larger than the diameter of the sun.
  • The idea is to move the telescope with the sun
    until it precisely aligned in the circular hair.
    At that moment, you stop moving the telescope and
    get the precise UTC time.

15
Solar ObservationsStep 3 Direct Vertical
Circle Left
  • With the vertical circle on the left, find the
    sun as described in Step 2 above.
  • Align the sun in the circular hair. At the
    moment it is aligned, note the time and record it
    on the observation form.
  • Record the horizontal circle reading on the
    observation form.
  • Make three more observations on the sun with the
    vertical circle left. Record the time and
    horizontal angle on the observation form.

16
Solar ObservationsStep 4 Reverse Vertical
circle right
  • Remove the solar filter and eyepiece, rotate the
    theodolite 180 so that the vertical circle is on
    the right and find the sun as described in Step 2
    above.
  • Align the sun in the circular hair. At the
    moment it is aligned, note the time and record it
    on the observation form.
  • Make three more observations on the sun with the
    vertical circle right and record the time and
    horizontal angle on the observation form.

17
Solar ObservationsStep 5 Sight on the azimuth
mark
  • Place the vertical circle on the right with the
    telescope aimed at the azimuth mark.
  • Precisely align the cross hairs with the azimuth
    mark.
  • Record the horizontal circle reading on the
    observation form.
  • Rotate the theodolite 180 so that the vertical
    circle is on the left with the telescope aimed at
    the azimuth mark.
  • Precisely align the cross lines with the azimuth
    mark.
  • Record the horizontal circle reading on the
    observation form.

18
Computation of the Azimuth
  • The simplest computation method is to use a
    computer program.
  • Elgin, Knowles and Senne, Inc. has several
    products for comuter or HP 48 calculator
    http//www.rollanet.org/eksi/
  • A freeware program is available from
  • http//www3.sympatico.ca/craymer/spade/

19
Computation (cont.)
  • The procedure and formulas are also described in
    the Sokkia Celestial Observation handbook and
    Ephemeris, which is printed yearly.
  • A Naval Almanac is available from
    http//aa.usno.navy.mil/publications/docs/ord_info
    .php

20
Azimuth Determination From Solar Observations
  • ALAN M BERARDUCCI
  • National Geomagnetism Program
  • US Geological Survey
  • geomag.usgs.gov
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