There is a very nice program for calculating local geomagnetic deviation
available from the NOAA National Geophysical Data Center, known as the
Geomagnetic Field Synthesis Program. The source is available for
download and the website given below also allows the program to be
executed without source download.

http://www.ngdc.noaa.gov/cgi-bin/seg/gmag/fldsnth1.pl

I use this program to determine the deviation for a specific site for
solar eclipse observation. Among other camera systems, I set up a
time-lapse video camera on a clock-driven polar equatorial mount. Since
this is done during the daylight hours, I use a good magnetic compass
and the deviation value from the above website to set the right
ascension axis of the polar mount to the azimuth of true north. I use a
precision level and protractor to set the elevation angle. While not
perfect, the alignment has been adequate for a four-hour observation.

The website program also provides for calculating the change in
deviation over a period of time; dates from 1900 to 2000 are supported
now. Below is an example of the program output for my home location over
the past ten years.

(You may need to widen your mail viewer window to see the full width)

Model: DGRF90 
  Latitude: 33.84 deg
  Longitude: -117.87 deg
  Elevation: 287.00 ft
  Range of Interest: 1/1/1990 - 12/31/1999, step 1.00

 
--------------------------------------------------------------------------
   Date         D            I          H       X       Y       Z      
F
   (yr)       (deg)        (deg)       (nt)    (nt)    (nt)    (nt)   
(nt)
  1990.00   13d  51.8m   59d   1.0m   25248   24513    6049   42047  
49045
  1991.00   13d  50.5m   59d   0.1m   25231   24498    6036   41994  
48991
  1992.00   13d  49.2m   58d  59.3m   25213   24484    6023   41942  
48937
  1993.00   13d  47.9m   58d  58.4m   25196   24469    6010   41890  
48883
  1994.00   13d  46.6m   58d  57.5m   25179   24455    5996   41837  
48830
  1995.00   13d  45.3m   58d  56.7m   25162   24440    5983   41785  
48776
  1996.00   13d  44.7m   58d  55.9m   25141   24421    5974   41729  
48717
  1997.00   13d  44.1m   58d  55.1m   25120   24401    5965   41673  
48658
  1998.00   13d  43.5m   58d  54.4m   25099   24382    5955   41617  
48599
  1999.00   13d  42.9m   58d  53.6m   25078   24363    5946   41561  
48541
  - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
- - 
  2000.00   13d  42.4m   58d  52.8m   25057   24343    5937   41505  
48482
  - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
- - 
              dD        dI       dH       dX       dY       dZ        dF
           (min/yr)  (min/yr)  (nT/yr)  (nT/yr)  (nT/yr)  (nT/yr)  
(nT/yr)
  2000.00     -0.6     -0.8    -21.0    -19.4     -9.2     -56.1   
-58.9
 
--------------------------------------------------------------------------

The website has a very good explanation of the model and of each
parameter in the table above. There is also a link to a website that can
provide local coordinates.

I don't present this as the perfect solution to the magnetic north
thread seen on this reflector recently. Every approach has its
limitations and the best selection certainly depends on the application.
This has worked for me for my solar eclipse observing in some very
strange and remote parts of our Earth.
-- 
Best wishes,

Larry McDavid W6FUB
Anaheim, CA  (20 miles southeast of Los Angeles, near Disneyland)

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