| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67.81 | 220.35 | 40.94 | 133.55 | 16.56 | 50.19 | 29.01 | 305.96 | 0.5757 | -348.0 | -302.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.34 | 0.00 | 0.88 | 19.49 | 56.04 | 34.86 | 305.21 | 0.6618 | 625.0 | 530.0 | |
| 0.00 | 1.70 | 0.00 | 1.06 | 17.21 | 53.05 | 31.87 | 304.36 | 0.6133 | 396.0 | 231.4 | |
| 5.73 | 142.70 | 3.54 | 87.42 | 16.57 | 52.23 | 31.05 | 304.11 | 0.5993 | -804.9 | -421.9 | |
| 0.00 | 1.97 | 0.00 | 1.21 | 16.91 | 51.85 | 30.67 | 304.91 | 0.5973 | 12.0 | -65.5 | |
| 21.47 | -3.00 | 13.16 | -3.00 | 16.48 | 51.55 | 30.37 | 304.54 | 0.5908 | -907.2 | 999999 | |
| 0.81 | -3.00 | 0.49 | -3.00 | 16.37 | 51.06 | 29.88 | 304.80 | 0.5842 | -944.2 | 999999 | |
| 3.40 | 11.27 | 2.06 | 6.82 | 15.98 | 50.81 | 29.63 | 304.43 | 0.5784 | -799.5 | -658.2 | |
| 2.33 | -3.00 | 1.42 | -3.00 | 16.62 | 50.88 | 29.70 | 305.32 | 0.5840 | -756.5 | 999999 | |
| 1.25 | 2.06 | 0.76 | 1.25 | 16.43 | 50.70 | 29.52 | 305.18 | 0.5805 | -857.6 | -829.4 | |
| 3.31 | -3.00 | 2.01 | -3.00 | 16.55 | 50.43 | 29.25 | 305.59 | 0.5783 | -800.6 | 999999 | |
| 0.00 | 1.79 | 0.00 | 1.08 | 15.99 | 50.27 | 29.09 | 304.92 | 0.5722 | -741.0 | -580.0 | |
| 4.83 | -3.00 | 2.92 | -3.00 | 16.38 | 50.26 | 29.08 | 305.50 | 0.5750 | -896.1 | 999999 | |
| 7.96 | 10.20 | 4.79 | 6.13 | 15.73 | 50.12 | 28.94 | 304.66 | 0.5685 | -987.6 | -782.4 | |
| 0.98 | -3.00 | 0.60 | -3.00 | 16.60 | 50.23 | 29.05 | 305.86 | 0.5763 | -777.0 | 999999 | |
| 0.63 | 2.68 | 0.38 | 1.61 | 16.04 | 49.81 | 28.63 | 305.41 | 0.5672 | -806.3 | -638.7 | |
| 0.00 | 1.07 | 0.00 | 0.64 | 16.10 | 49.53 | 28.35 | 305.75 | 0.5643 | -769.0 | -722.5 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 14.82 | 49.30 | 28.13 | 303.99 | 0.5518 | -665.0 | -535.6 | |
| 0.00 | 1.34 | 0.00 | 0.80 | 16.15 | 49.08 | 27.90 | 306.25 | 0.5594 | -854.0 | -718.1 | |
| 0.00 | 1.43 | 0.00 | 0.88 | 19.62 | 49.10 | 27.92 | 311.20 | 0.5883 | -608.0 | -332.2 | |
| 0.00 | 1.07 | 0.00 | 0.66 | 19.89 | 49.15 | 27.97 | 311.51 | 0.5911 | -458.0 | -397.4 | |
| 2.59 | 3.94 | 1.58 | 2.40 | 19.58 | 48.80 | 27.62 | 311.43 | 0.5847 | -733.2 | -718.5 | |
| 1.25 | 2.24 | 0.77 | 1.37 | 19.98 | 48.87 | 27.69 | 311.90 | 0.5890 | -557.1 | -465.5 | |
| 0.00 | 1.25 | 0.00 | 0.76 | 19.87 | 48.56 | 27.38 | 312.06 | 0.5847 | -666.0 | -522.8 | |
| 0.00 | 0.36 | 0.00 | 0.21 | 15.92 | 47.87 | 26.69 | 307.07 | 0.5434 | 421.0 | 507.0 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 15.79 | 47.85 | 26.67 | 306.89 | 0.5422 | 556.0 | 501.4 | |
| 0.00 | 1.34 | 0.00 | 0.79 | 15.79 | 47.64 | 26.46 | 307.09 | 0.5396 | 651.0 | 471.8 | |
| 0.00 | 1.07 | 0.00 | 0.64 | 17.36 | 47.34 | 26.16 | 309.75 | 0.5495 | 594.0 | 443.2 | |
| 1.16 | 2.33 | 0.68 | 1.36 | 16.46 | 46.26 | 25.08 | 309.55 | 0.5294 | 746.3 | 661.2 | |
| 0.00 | 0.98 | 0.00 | 0.57 | 16.89 | 45.73 | 24.55 | 310.80 | 0.5273 | 656.0 | 548.6 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 17.38 | 44.69 | 23.51 | 312.73 | 0.5203 | 680.0 | 559.3 | |
| 0.00 | 1.52 | 0.00 | 0.87 | 15.80 | 44.45 | 23.27 | 310.59 | 0.5026 | 708.0 | 556.2 | |
| 0.00 | 1.16 | 0.00 | 0.67 | 16.76 | 44.40 | 23.22 | 312.14 | 0.5111 | 651.0 | 533.2 | |
| 0.00 | 1.52 | 0.00 | 0.87 | 16.56 | 44.06 | 22.89 | 312.23 | 0.5055 | 715.0 | 592.2 | |
| 10.11 | 16.64 | 5.78 | 9.52 | 16.20 | 43.95 | 22.77 | 311.82 | 0.5008 | 1013.9 | 714.6 | |
| 0.00 | 0.72 | 0.00 | 0.41 | 18.10 | 43.65 | 22.47 | 315.04 | 0.5161 | 663.0 | 637.2 | |
| 0.00 | 2.51 | 0.00 | 1.41 | 14.97 | 43.03 | 21.85 | 311.00 | 0.4783 | 506.0 | 587.1 | |
| 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. | |