| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.73 | 21.71 | 0.40 | 11.79 | -13.65 | 256.75 | 17.08 | 224.09 | 0.4117 | 576.9 | 542.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.27 | 0.00 | 1.25 | -13.25 | 259.75 | 20.09 | 229.57 | 0.4410 | 604.0 | 535.8 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -13.41 | 259.60 | 19.93 | 229.08 | 0.4407 | 901.0 | 794.8 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -13.65 | 259.12 | 19.46 | 227.97 | 0.4376 | 646.0 | 572.7 | |
| 0.00 | 1.91 | 0.00 | 1.05 | -13.36 | 258.86 | 19.20 | 228.11 | 0.4316 | 879.0 | 728.9 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -14.18 | 258.73 | 19.07 | 226.48 | 0.4386 | 663.0 | 551.5 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -13.93 | 258.67 | 19.01 | 226.84 | 0.4353 | 714.0 | 656.8 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -13.25 | 256.74 | 17.08 | 225.00 | 0.4060 | 747.0 | 691.1 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -11.79 | 256.48 | 16.82 | 227.30 | 0.3870 | 822.0 | 678.5 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -11.94 | 256.36 | 16.70 | 226.80 | 0.3873 | 907.0 | 772.1 | |
| 0.73 | 5.63 | 0.40 | 3.06 | -14.77 | 255.84 | 16.17 | 220.86 | 0.4134 | 976.2 | 705.8 | |
| 0.00 | 0.55 | 0.00 | 0.29 | -12.00 | 254.32 | 14.66 | 222.99 | 0.3646 | 763.0 | 572.3 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -11.38 | 253.26 | 13.60 | 222.07 | 0.3456 | 782.0 | 502.5 | |
| 0.00 | 0.82 | 0.00 | 0.44 | -15.96 | 252.56 | 12.89 | 212.87 | 0.3970 | -811.0 | -717.6 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -14.62 | 250.57 | 10.91 | 210.56 | 0.3618 | -677.0 | -579.9 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |