Sunspot Cycle
Observations over many years reveal a 22 year cycle of activity in
the photosphere.

The number of sunspots reaches a maximum about every 11 years,
but successive maxima have spots with reversed magnetic polarity.
Thus the whole cycle is 22 years long.
The record of observations indicates that this cycle has been going
on back to the early 1700's, although the strength of the cycle
varies. For the period 1645 to 1715 the record is rather spotty, but
suggests that there were hardly any sunspots.

The luminosity of the Sun increases a little when there are sunspots.
During the period 1645 to 1715 the Earth was unusually cold.
There is a model for how this works. The model makes use of the observation
that the upper layers of the Sun rotate faster near the Sun's equator than
near its poles. The idea is that the magnetic field gets concentrated along
long lines underneath the photosphere and that these likes get stretched out
by the differential rotation.

If the field comes out of the photosphere, that makes a pair of sunspots.

An analysis of this model in its details is enormously difficult. But
we can ask a few critical questions:
- Does the differential rotation provide the right timescale?
- At 30 degrees north or south of the equator, it takes 27.5 days for the
photosphere to rotate once. Thus this part of the photosphere rotates
365/27.5 = 13.3 times around in a year.
- At the equator, it takes 25.0 days for the
photosphere to rotate once. Thus this part of the photosphere rotates
365/25.0 = 14.6 times around in a year.
- Thus the equator moves 14.6 - 13.3 = 1.3 times around relative the
the area at 30 degrees.
- That's roughly one wrapping per year, enough to cause quite a tangle
in the 5.5 years from a sunspot minimum to a sunspot maximum.
- There is a simple prediction: sunspot pairs should be oriented
east-west on the Sun's surface.
- There is another simple prediction:
- At any one time, in the Sun's northern hemisphere, the eastern spots in sunspot pairs should always
have the same magnetic polarity (call it N).
- The polarity for sunspot pairs in the Sun's southern hemisphere should
be the opposite (in this case S).
Good scientists that we are, we can check these predictions against the
1995 Jul 09 magnetogram that we looked at before. (Recall that white
represents one polarity, black the opposite polarity.)
Davison E. Soper, Institute of Theoretical Science,
University of Oregon, Eugene OR 97403 USA
soper@bovine.uoregon.edu