| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.06 | 23.93 | 0.52 | 11.91 | -7.54 | 8.21 | -4.28 | 138.44 | 0.0876 | -65.8 | -128.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.76 | 0.00 | 0.87 | -7.18 | 12.95 | 0.46 | 205.68 | 0.0186 | 893.0 | 605.2 | |
| 0.00 | 1.58 | 0.00 | 0.79 | -4.51 | 12.89 | 0.41 | 346.71 | 0.0308 | 1002.0 | 723.9 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -8.26 | 12.80 | 0.31 | 188.64 | 0.0361 | 894.0 | 726.2 | |
| 0.00 | 2.55 | 0.00 | 1.27 | -7.27 | 11.13 | -1.35 | 128.00 | 0.0298 | 900.0 | 682.9 | |
| 0.00 | 0.79 | 0.00 | 0.39 | -7.39 | 10.68 | -1.80 | 123.09 | 0.0374 | 816.0 | 636.3 | |
| 0.00 | 1.50 | 0.00 | 0.74 | -10.12 | 10.33 | -2.16 | 151.41 | 0.0778 | 1105.0 | 911.1 | |
| 1.06 | 2.20 | 0.52 | 1.09 | -9.73 | 10.03 | -2.46 | 145.35 | 0.0747 | 1088.3 | 938.5 | |
| 0.00 | 1.06 | 0.00 | 0.53 | -7.23 | 6.29 | -6.20 | 99.62 | 0.1091 | -806.0 | -647.0 | |
| 0.00 | 1.14 | 0.00 | 0.57 | -7.10 | 5.71 | -6.77 | 97.81 | 0.1187 | -943.0 | -735.3 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -7.34 | 5.49 | -6.99 | 99.51 | 0.1230 | -1128.0 | -922.6 | |
| 0.00 | 2.20 | 0.00 | 1.10 | -6.95 | 5.32 | -7.17 | 96.19 | 0.1252 | -1152.0 | -919.4 | |
| 0.00 | 1.14 | 0.00 | 0.57 | -7.39 | 5.22 | -7.27 | 99.62 | 0.1278 | -1124.0 | -819.9 | |
| 0.00 | 2.29 | 0.00 | 1.14 | -7.27 | 4.98 | -7.51 | 98.41 | 0.1316 | -1021.0 | -879.4 | |
| 0.00 | 3.34 | 0.00 | 1.67 | -7.57 | 4.85 | -7.64 | 100.50 | 0.1346 | -892.0 | -841.3 | |
| 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. | |