| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.04 | 357.77 | 73.28 | 341.38 | 15.53 | 88.21 | 59.44 | 283.84 | 0.8565 | 492.1 | 211.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.54 | 209.71 | 34.26 | 201.87 | 14.86 | 88.60 | 59.82 | 283.05 | 0.8598 | 901.2 | 275.9 | |
| 0.00 | 2.04 | 0.00 | 1.91 | 12.30 | 87.43 | 58.65 | 280.04 | 0.8495 | -467.0 | -346.8 | |
| 0.00 | 1.24 | 0.00 | 1.16 | 12.48 | 87.49 | 58.72 | 280.25 | 0.8500 | -259.0 | -215.6 | |
| 0.00 | 1.16 | 0.00 | 1.08 | 12.61 | 87.36 | 58.59 | 280.41 | 0.8489 | -264.0 | -260.2 | |
| 0.80 | 1.87 | 0.74 | 1.72 | 12.37 | 87.09 | 58.32 | 280.11 | 0.8464 | -480.8 | -387.4 | |
| 10.66 | 42.30 | 10.39 | 41.36 | 16.78 | 88.92 | 60.15 | 285.28 | 0.8628 | -104.2 | 184.4 | |
| 0.00 | 1.95 | 0.00 | 1.79 | 12.50 | 86.73 | 57.95 | 280.26 | 0.8431 | -480.0 | -425.1 | |
| 0.00 | 1.16 | 0.00 | 1.05 | 12.02 | 86.33 | 57.55 | 279.69 | 0.8394 | -594.0 | -515.4 | |
| 0.00 | 1.07 | 0.00 | 0.96 | 12.49 | 86.20 | 57.43 | 280.25 | 0.8382 | -598.0 | -471.8 | |
| 0.00 | 2.67 | 0.00 | 2.61 | 18.68 | 89.03 | 60.26 | 287.48 | 0.8643 | -362.0 | -220.4 | |
| 3.73 | 44.87 | 3.55 | 42.53 | 17.22 | 88.02 | 59.25 | 285.82 | 0.8552 | 555.3 | 147.7 | |
| 0.00 | 1.69 | 0.00 | 1.55 | 15.69 | 86.85 | 58.07 | 284.06 | 0.8444 | 568.0 | 421.4 | |
| 8.89 | -11.00 | 8.36 | -11.00 | 17.54 | 87.69 | 58.92 | 286.21 | 0.8525 | 766.1 | 999999 | |
| 7.20 | 20.88 | 6.67 | 19.28 | 16.51 | 87.11 | 58.33 | 285.02 | 0.8470 | 637.5 | 473.9 | |
| 2.40 | -14.00 | 2.20 | -14.00 | 16.29 | 86.82 | 58.05 | 284.77 | 0.8444 | 762.5 | 999999 | |
| 7.20 | 9.86 | 6.52 | 8.94 | 15.56 | 86.31 | 57.54 | 283.92 | 0.8395 | 674.5 | 377.5 | |
| 0.62 | 3.73 | 0.59 | 3.52 | 19.00 | 87.82 | 59.05 | 287.92 | 0.8542 | -584.6 | -448.1 | |
| 0.00 | 0.80 | 0.00 | 0.72 | 15.85 | 85.97 | 57.20 | 284.27 | 0.8365 | 591.0 | 509.6 | |
| 0.00 | 1.69 | 0.00 | 1.52 | 16.04 | 85.94 | 57.16 | 284.50 | 0.8362 | 224.0 | 223.2 | |
| 0.00 | 2.58 | 0.00 | 2.24 | 13.89 | 84.61 | 55.83 | 281.94 | 0.8231 | -433.0 | -328.2 | |
| 0.00 | 1.42 | 0.00 | 1.22 | 13.38 | 84.15 | 55.37 | 281.33 | 0.8186 | -551.0 | -498.8 | |
| 0.00 | 1.07 | 0.00 | 0.91 | 13.22 | 83.87 | 55.10 | 281.14 | 0.8159 | -614.0 | -543.6 | |
| 0.00 | 0.62 | 0.00 | 0.55 | 17.03 | 85.35 | 56.58 | 285.73 | 0.8312 | 415.0 | 393.0 | |
| 0.00 | 0.27 | 0.00 | 0.24 | 17.63 | 85.58 | 56.81 | 286.43 | 0.8336 | 511.0 | 550.0 | |
| 0.00 | 1.07 | 0.00 | 0.91 | 13.54 | 83.77 | 54.99 | 281.53 | 0.8149 | -611.0 | -534.2 | |
| 0.00 | 1.07 | 0.00 | 0.94 | 17.29 | 85.25 | 56.47 | 286.05 | 0.8303 | 498.0 | 409.2 | |
| 0.00 | 0.98 | 0.00 | 0.80 | 14.69 | 81.88 | 53.10 | 283.02 | 0.7962 | -451.0 | -347.3 | |
| 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. | |