In a message dated 02/03/2000 10:19:54 AM Eastern Standard Time,
roybar@........ writes:
<< Is there a link to construction details, etc. about McWilliams
magnetometer?
Bob >>
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Hi Bob,
There is no link but I can tell you briefly how it works. Later I could
send you detailed drawings and instructions how to build it. These are from
the August 1998 Solar Bulletin published by the American Association of
Variable Star Observers (AAVSO). I would need a postal address or FAX number.
The basic design is a torsion magnetometer consisting of a bar magnet
suspended on a torsion wire that can be a piece of guitar string 0.2 mm
diameter and about 25-40 cm long. The bar magnet should be about 6 mm
diameter and 5 cm long. The magnet is mounted with epoxy in the middle of a
thin wooden vane about
1cm wide and 20cm long. The torsion wire can be epoxied to the center of the
magnet so the vane hangs horizontal. The upper mount for the torsion wire is
then rotated to provide enough torque to make the wooden vane point east and
west instead of its preferred north-south direction that it seeks as a
compass. The vane is now torsion balanced against the Earths magnetic field
and will rotate in response to changes in the strength of the field due to
magnetic storms. Beneath one end of the wooden vane are two Radio Shack
photocells and above it is a 12-volt automobile bulb, the kind with a
straight filament. The bulb and the photocells are arranged so the shadow
vane shades one half of each photocell from the lamp above. The linear design
of the photocells should be oriented so the lines are perpendicular to the
edge of the shadow vane. The photocells are variable resistors. their
resistance varies in direct relation to how much light falls on them. If they
are equally shaded their resistance is equal. They are made two legs of a
four-leg Wheatstone bridge. The other two legs can be 5000 ohm 1/4 Watt
resistors. A regulated 9-volt power supply is connected across the bridge and
also lights the 12-volt automobile lamp (9-volts is plenty for this
application). A chart recorder or A/D converter and computer is connected
between the centers of the two legs of the bridge. The two resistors in
series have 9-volts across them but at the center the voltage is half as much
or 4 1/2-volts. There is also 9-volts across the two photocells that are also
connected in series. At the center where they are connected together the
voltage is also 4 1/2-volts provided the shadow vane shades the photocells
equally which is the way it should be set initially. The recorder is
connected between these two 4 1/2-volt points and since they are of equal
potential, no current flows and the recorder reads zero (adjust it or bias it
so the zero point is in the middle of the chart). When the strength of the
Earth's magnetic field changes in response to a solar flare of coronal mass
ejection, the shadow vane's balance by the torsion wire becomes unbalanced
and rotates the position of the shadow vane above the photocells. this
increases the resistance of one photocell and lowers the resistance of the
other and unbalances the Wheatstone bridge so current flows in the recorder.
It moves it up or down depending on whether the flare-induced current in the
Earth's magnetosphere adds to or subtracts from the normal earth magnetic
field strength.
The beautiful part of the McWilliams magnetometer is its simplicity. It
produces recordings equal to those of professional flux gate magnetometers at
the USGS magnetic observatories. Furthermore it needs no amplification and
can easily drive a 0 to 1 milliamp recorder directly and is sensitive enough
to spread a magnetic storm over the full chart. Most AAVSO magnetic storm
observers use Rustrak strip chart recorders running 1/4 inch/hr but it can
also be recorded on a computer using Windaq. For details on recording with
Windaq email Jerry Winkler at . He will be glad to help
you. I should mention that the shadow vane must be damped like a seismograph
and for the same reason. A damper in an oil cup under the shadow vane will do
the trick. Don't use magnetic damping for obvious reasons and place it as far
as possible from big steel objects. Place the magnetometer far from
driveways. Cars passing by at a distance of ~40m will put tiny blips on the
chart but moving a car in your driveway will send it off scale. The
McWilliams photocell sensor would probably work quite well on a seismograph.
Have fun,
Cap
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Larry Cochrane <cochrane@..............>