| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.24 | 54.01 | 17.20 | 47.92 | -7.84 | 249.42 | 54.35 | 256.20 | 0.8305 | 137.3 | 206.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.08 | 2.62 | 1.09 | 2.64 | -6.69 | 254.36 | 59.29 | 258.73 | 0.8727 | 515.0 | 382.7 | |
| 0.00 | 0.99 | 0.00 | 0.94 | -3.00 | 252.91 | 57.84 | 262.65 | 0.8544 | 399.0 | 394.8 | |
| 0.00 | 1.08 | 0.00 | 1.05 | -6.78 | 253.02 | 57.95 | 258.33 | 0.8614 | 407.0 | 364.1 | |
| 0.00 | 0.54 | 0.00 | 0.51 | -6.31 | 251.90 | 56.83 | 258.62 | 0.8507 | 411.0 | 377.5 | |
| 0.00 | 0.54 | 0.00 | 0.50 | -8.52 | 250.61 | 55.54 | 255.74 | 0.8435 | 49.0 | 63.8 | |
| 0.00 | 0.81 | 0.00 | 0.73 | -7.62 | 249.94 | 54.87 | 256.61 | 0.8354 | 466.0 | 449.9 | |
| 0.00 | 0.81 | 0.00 | 0.73 | -7.77 | 249.91 | 54.85 | 256.43 | 0.8355 | 588.0 | 412.6 | |
| 0.00 | 1.17 | 0.00 | 1.06 | -8.21 | 249.95 | 54.88 | 255.92 | 0.8367 | 424.0 | 340.0 | |
| 11.02 | 22.32 | 9.71 | 19.64 | -6.74 | 249.46 | 54.39 | 257.53 | 0.8291 | 655.5 | 452.9 | |
| 0.00 | 3.79 | 0.00 | 3.43 | -9.02 | 249.91 | 54.84 | 254.97 | 0.8381 | 532.0 | 450.0 | |
| 0.00 | 2.44 | 0.00 | 2.19 | -9.32 | 249.71 | 54.64 | 254.57 | 0.8370 | 162.0 | 141.1 | |
| 0.00 | 1.54 | 0.00 | 1.41 | -11.11 | 250.06 | 54.99 | 252.60 | 0.8443 | -421.0 | -305.8 | |
| 7.14 | 10.12 | 6.40 | 9.08 | -9.67 | 249.47 | 54.40 | 254.09 | 0.8356 | -621.3 | -341.5 | |
| 0.00 | 0.72 | 0.00 | 0.61 | -8.40 | 247.13 | 52.06 | 254.91 | 0.8102 | 596.0 | 560.1 | |
| 0.00 | 0.81 | 0.00 | 0.64 | -11.06 | 243.64 | 48.57 | 250.53 | 0.7828 | -547.0 | -489.3 | |
| 0.00 | 1.45 | 0.00 | 1.14 | -11.19 | 243.30 | 48.23 | 250.24 | 0.7797 | -588.0 | -523.1 | |
| 0.00 | 1.36 | 0.00 | 1.01 | -8.58 | 241.03 | 45.96 | 252.66 | 0.7470 | -393.0 | -329.9 | |
| 0.00 | 0.90 | 0.00 | 0.61 | 0.13 | 237.50 | 42.43 | 263.50 | 0.6813 | -612.0 | -509.3 | |
| 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. | |