All Figures

	Figure 1: Finding chart for SS UMi covering a region of  arcmin. The positions of the comparison stars are shown. North is up, East is left.
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In the text

Figure 2: The general photometric behavior of SS UMi during the whole 2004 campaign. Visual estimates collected by AAVSO observers are shown as open circles and the CCD observations described in this paper as black dots. The open triangles correspond to the "fainter than'' estimates from AAVSO. Big filled triangles point to the expected positions of superoutbursts assuming 84.7 days supercycle length. Two arrows show the moments of maximum magnitude of the recorded superoutbursts.

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In the text

	Figure 3: The light curves of SS UMi during its April 2004 superoutburst.
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In the text

	Figure 4: The ANOVA power spectrum of the light curve of SS UMi from its 2004 April superoutburst.
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In the text

	Figure 5: The O-C diagram for the superhump maxima of SS UMi during its April 2004 superoutburst. The solid line corresponds to the fit resulting from the ephemeris (2).
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In the text

	Figure 6: The dependences between supercycle length and mass transfer in normal SU UMa stars and ER UMa variables.
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In the text

	Figure 7: The Kukarkin-Parenago relation between amplitude of the outburst and cycle length for dwarf novae. The filled and open circles denote the positions of SS UMi for 1999-2000 and 2004, respectively.
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In the text

	Figure 8: The relation between amplitude supercycle and cycle lengths for dwarf novae. The filled and open circles denote the positions of SS UMi for 1999-2000 and 2004, respectively.
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In the text