Running the code with different number of BMRs per cycle

The code was run with different values of input BMRs per cycle, and the initial field was varied for each run to get a stable oscillation. The results are:

1. No. of BMRs per cycle = 7028,  with a peak of 200 BMRs@5.5 yrs.

Initial field = 3.5G
The field oscillates between +2.65G and -2.55G
Difference=5.20G

2. No. of BMRs per cycle = 10722, with a peak of 300 BMRs@5.5 yrs.

Initial field = 5G
The field oscillates between +3.81G and -3.64G
Difference=7.45G

3. No. of BMRs per cycle = 14412, with a peak of 400 BMRs@5.5 yrs.

Initial field = 7G
The field oscillates between +5.31 and -5.10
Difference= 10.41G

4. No. of BMRs per cycle = 18082, with a peak of 500 BMRs@5.5 yrs.

Initial field = 10G
The field oscillates between +6.58 and -7.25
Difference=15.85G

5. No. of BMRs per cycle = 21768, with a peak of 600 BMRs@5.5yrs.

Initial field = 12G
The field oscillates between +8.66 and -8.66G
Difference=17.32G


6. No. of BMRs per cycle = 25442, with a peak of 700 BMRs@5.5yrs.

Initial field = 13.5G
The field oscillates between +10.14 and -9.75G
Difference=19.89G


Ideally, the Sun's peak magnetic field near the poles has a magnitude of about 10G. So, keeping the separation between 2 spots in a BMR to be minimum, so that they just grace each other, we obtain a field of about 10 G in the last case.