| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.07 | 36.69 | 5.17 | 18.81 | 16.02 | 23.10 | 6.93 | 332.90 | 0.2606 | -9.6 | -67.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.90 | 6.36 | 2.51 | 3.26 | 13.51 | 26.66 | 10.50 | 316.24 | 0.2573 | 1049.6 | 841.0 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 15.08 | 25.39 | 9.23 | 323.81 | 0.2634 | -783.0 | -508.5 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 15.70 | 25.23 | 9.06 | 325.69 | 0.2703 | -786.0 | -632.8 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 16.36 | 25.26 | 9.10 | 326.99 | 0.2796 | -892.0 | -774.7 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.36 | 25.05 | 8.89 | 325.45 | 0.2639 | -840.0 | -633.0 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.55 | 24.80 | 8.64 | 326.61 | 0.2642 | -968.0 | -771.5 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 16.52 | 24.65 | 8.49 | 329.05 | 0.2765 | -882.0 | -679.6 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 14.50 | 23.71 | 7.55 | 327.74 | 0.2394 | -943.0 | -678.8 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 16.56 | 23.63 | 7.47 | 332.24 | 0.2686 | -1144.0 | -987.8 | |
| 0.00 | 2.27 | 0.00 | 1.16 | 16.10 | 22.56 | 6.39 | 334.92 | 0.2536 | -892.0 | -628.6 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 16.51 | 21.77 | 5.61 | 338.31 | 0.2547 | -953.0 | -642.2 | |
| 1.36 | 1.82 | 0.70 | 0.93 | 17.48 | 20.97 | 4.80 | 342.41 | 0.2656 | 810.0 | 706.6 | |
| 3.81 | 6.08 | 1.96 | 3.12 | 17.11 | 20.89 | 4.73 | 342.21 | 0.2592 | 1091.2 | 532.5 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 17.61 | 20.75 | 4.58 | 343.32 | 0.2665 | 520.0 | 467.8 | |
| 0.00 | 3.27 | 0.00 | 1.67 | 16.51 | 20.69 | 4.52 | 342.20 | 0.2485 | 1138.0 | 819.6 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 17.49 | 20.55 | 4.39 | 343.85 | 0.2636 | 1031.0 | 833.2 | |
| 0.00 | 2.27 | 0.00 | 1.17 | 18.28 | 20.35 | 4.18 | 345.37 | 0.2755 | 869.0 | 602.4 | |
| 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. | |