| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 93.07 | 525.95 | 66.27 | 364.97 | 11.76 | 260.51 | -39.92 | 64.37 | 0.6941 | -629.0 | -260.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.78 | 0.00 | 0.53 | 14.03 | 262.87 | -37.56 | 60.38 | 0.6827 | 429.0 | 372.8 | |
| 0.00 | 1.30 | 0.00 | 0.88 | 14.20 | 262.68 | -37.75 | 60.28 | 0.6858 | 512.0 | 412.5 | |
| 78.03 | 469.21 | 51.86 | 312.39 | 11.96 | 263.04 | -37.39 | 63.02 | 0.6689 | -1103.2 | -327.9 | |
| 0.35 | 2.35 | 0.24 | 1.61 | 13.52 | 261.67 | -38.76 | 61.80 | 0.6930 | -526.2 | -408.9 | |
| 0.00 | 0.78 | 0.00 | 0.54 | 10.71 | 259.67 | -40.76 | 66.65 | 0.7011 | -501.0 | -362.1 | |
| 0.00 | 0.78 | 0.00 | 0.57 | 11.45 | 257.20 | -43.23 | 66.93 | 0.7320 | -475.0 | -395.2 | |
| 0.00 | 1.30 | 0.00 | 0.95 | 11.58 | 256.84 | -43.59 | 66.95 | 0.7365 | -514.0 | -379.5 | |
| 0.00 | 0.96 | 0.00 | 0.83 | 16.50 | 250.12 | -50.30 | 64.11 | 0.8222 | -367.0 | -305.0 | |
| 0.00 | 0.96 | 0.00 | 0.81 | 14.09 | 250.29 | -50.14 | 66.81 | 0.8122 | 631.0 | 516.0 | |
| 0.00 | 1.04 | 0.00 | 0.95 | 9.58 | 245.78 | -54.64 | 73.63 | 0.8403 | 371.0 | 295.2 | |
| 6.78 | 44.84 | 6.53 | 43.25 | 10.23 | 243.78 | -56.65 | 73.50 | 0.8594 | 664.8 | 270.6 | |
| 0.00 | 0.43 | 0.00 | 0.42 | 10.60 | 243.51 | -56.92 | 73.16 | 0.8625 | 165.0 | 219.2 | |
| 7.91 | -11.00 | 7.64 | -11.00 | 9.95 | 243.52 | -56.90 | 73.89 | 0.8609 | 607.0 | 999999 | |
| 0.00 | 1.22 | 0.00 | 1.24 | 12.04 | 242.25 | -58.17 | 71.92 | 0.8761 | 34.0 | 86.4 | |
| 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. | |