Abstract
The images of sunspots in sixteen active regions taken at the UCCI Observatory in Grand Cayman during June - November 2015, were used to determine their fractal dimensions using the perimeter-area method for the umbral and the penumbral region. Scale free fractal dimensions of 2.09 $\pm$ 0.42 and 1.72 $\pm$ 0.4 were found respectively. This value was higher than the value determined by Chumak and Chumak (1996) who used a similar method but for the penumbral region only for their sample set. There is a positive correlation r = 0.58 between umbral and the penumbral fractal dimensions for the specific sunspots. Furthermore, a time series analysis was done similarly on eight images of AR 12403, from 21st August 2015 - 28th August 2015 taken from the Debrecen Photoheliographic Data (DPD). The correlation, r = 0.623 between the umbral and penumbral fractal dimensions in the time series indicating that the complexity in morphology indicated by the fractal dimension between the umbra and penumbra followed each other in time as well.
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