| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 120 | 751 | 58 | 372 | 2.58 | 271.69 | 2.15 | 235.80 | 0.0455 | 1884.2 | 698.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41 | 675 | 20 | 335 | 2.12 | 273.06 | 3.53 | 241.40 | 0.0704 | 2080.4 | 752.0 | |
| 15 | -1 | 7 | -1 | 2.00 | 272.60 | 3.07 | 236.37 | 0.0645 | 2071.4 | 999999 | |
| 7 | -1 | 3 | -1 | 3.20 | 272.37 | 2.84 | 253.40 | 0.0518 | 1605.2 | 999999 | |
| 5 | -1 | 3 | -1 | 2.58 | 272.33 | 2.80 | 242.41 | 0.0553 | 1561.7 | 999999 | |
| 32 | -1 | 16 | -1 | 2.89 | 271.95 | 2.41 | 244.44 | 0.0468 | 2103.6 | 999999 | |
| 8 | -1 | 4 | -1 | 2.27 | 271.94 | 2.41 | 233.73 | 0.0524 | 1491.6 | 999999 | |
| 7 | -1 | 3 | -1 | 3.43 | 271.75 | 2.22 | 254.52 | 0.0403 | 1516.2 | 999999 | |
| 0 | 5 | 0 | 2 | 0.12 | 271.33 | 1.79 | 204.57 | 0.0756 | 792.0 | 613.4 | |
| 5 | -1 | 2 | -1 | 2.78 | 271.29 | 1.76 | 234.16 | 0.0380 | 1429.2 | 999999 | |
| 0 | 10 | 0 | 5 | 3.35 | 266.51 | -3.02 | 102.90 | 0.0542 | 840.0 | 725.8 | |
| 0 | 18 | 0 | 9 | 2.89 | 266.13 | -3.41 | 108.72 | 0.0629 | 713.0 | 657.8 | |
| 0 | 6 | 0 | 3 | 2.34 | 265.09 | -4.45 | 110.85 | 0.0833 | 769.0 | 583.2 | |
| 0 | 14 | 0 | 7 | 1.45 | 264.70 | -4.83 | 118.10 | 0.0959 | 651.0 | 563.4 | |
| 0 | 7 | 0 | 3 | 5.91 | 264.13 | -5.40 | 70.61 | 0.0997 | -1004.0 | -839.3 | |
| 0 | 7 | 0 | 4 | 6.10 | 263.51 | -6.02 | 70.82 | 0.1110 | -1051.0 | -836.4 | |
| 0 | 3 | 0 | 1 | 6.45 | 263.51 | -6.03 | 67.91 | 0.1131 | -746.0 | -784.2 | |
| 0 | 6 | 0 | 3 | 4.83 | 259.55 | -9.99 | 85.10 | 0.1742 | -791.0 | -635.3 | |
| 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. | |