| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.69 | 35.08 | 0.94 | 19.74 | -17.05 | 157.81 | 14.61 | 210.46 | 0.4762 | 22.6 | 256.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.43 | 0.00 | 0.82 | -17.38 | 162.05 | 18.85 | 216.92 | 0.5153 | 884.0 | 693.9 | |
| 0.00 | 4.73 | 0.00 | 2.74 | -17.90 | 161.73 | 18.53 | 215.84 | 0.5186 | 851.0 | 756.3 | |
| 0.00 | 1.34 | 0.00 | 0.77 | -17.23 | 161.56 | 18.36 | 216.40 | 0.5092 | 827.0 | 681.3 | |
| 0.00 | 1.07 | 0.00 | 0.61 | -17.12 | 159.80 | 16.60 | 213.81 | 0.4926 | 658.0 | 643.1 | |
| 0.00 | 0.45 | 0.00 | 0.25 | -17.52 | 159.01 | 15.81 | 212.08 | 0.4911 | 483.0 | 409.2 | |
| 0.00 | 1.34 | 0.00 | 0.76 | -17.70 | 157.41 | 14.21 | 209.23 | 0.4811 | -766.0 | -656.0 | |
| 0.62 | 3.66 | 0.35 | 2.07 | -18.08 | 157.08 | 13.88 | 208.26 | 0.4838 | -919.7 | -768.1 | |
| 1.07 | 6.16 | 0.59 | 3.41 | -15.86 | 156.79 | 13.59 | 210.15 | 0.4518 | 1066.2 | 811.4 | |
| 0.00 | 1.87 | 0.00 | 1.04 | -16.52 | 156.84 | 13.64 | 209.49 | 0.4610 | 853.0 | 704.2 | |
| 0.00 | 1.25 | 0.00 | 0.70 | -17.84 | 156.84 | 13.64 | 208.08 | 0.4788 | -749.0 | -691.1 | |
| 0.00 | 4.46 | 0.00 | 2.48 | -16.08 | 156.64 | 13.44 | 209.63 | 0.4537 | 945.0 | 819.7 | |
| 0.00 | 1.43 | 0.00 | 0.80 | -16.90 | 156.47 | 13.27 | 208.42 | 0.4635 | 741.0 | 549.9 | |
| 0.00 | 1.25 | 0.00 | 0.71 | -19.66 | 155.96 | 12.76 | 204.83 | 0.4975 | -753.0 | -592.1 | |
| 0.00 | 1.34 | 0.00 | 0.74 | -16.41 | 155.60 | 12.40 | 207.33 | 0.4505 | -827.0 | -603.1 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -16.18 | 155.49 | 12.29 | 207.37 | 0.4465 | -617.0 | -559.0 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -19.49 | 155.72 | 12.52 | 204.56 | 0.4936 | -712.0 | -667.8 | |
| 0.00 | 1.52 | 0.00 | 0.84 | -16.13 | 154.84 | 11.64 | 206.18 | 0.4412 | -823.0 | -673.8 | |
| 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. | |