| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.06 | 284.08 | 24.15 | 152.77 | 5.78 | 45.71 | 20.27 | 296.68 | 0.3864 | -832.1 | -414.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.70 | 0.00 | 1.18 | 8.95 | 68.13 | 42.70 | 287.46 | 0.7046 | -663.0 | -552.7 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 11.46 | 60.25 | 34.81 | 294.89 | 0.6191 | -604.0 | -539.6 | |
| 0.00 | 1.36 | 0.00 | 0.86 | 11.79 | 60.00 | 34.56 | 295.53 | 0.6178 | -751.0 | -654.8 | |
| 0.85 | 6.89 | 0.49 | 3.97 | 10.18 | 52.48 | 27.05 | 298.52 | 0.5115 | -916.4 | -703.2 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 8.90 | 52.24 | 26.80 | 296.44 | 0.4996 | -751.0 | -675.3 | |
| 0.00 | 1.79 | 0.00 | 1.02 | 9.01 | 52.11 | 26.68 | 296.76 | 0.4987 | -800.0 | -613.7 | |
| 44.21 | 260.08 | 23.66 | 139.22 | 5.56 | 45.37 | 19.93 | 296.36 | 0.3803 | -1349.9 | -433.6 | |
| 0.00 | 2.47 | 0.00 | 1.32 | 8.52 | 43.49 | 18.05 | 305.63 | 0.3786 | -799.0 | -666.0 | |
| 0.00 | 1.28 | 0.00 | 0.66 | 2.85 | 39.73 | 14.29 | 296.59 | 0.2770 | 933.0 | 819.0 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 2.43 | 39.45 | 14.01 | 295.66 | 0.2696 | 919.0 | 690.9 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 3.71 | 38.28 | 12.85 | 302.05 | 0.2630 | 773.0 | 569.1 | |
| 0.00 | 0.77 | 0.00 | 0.39 | 5.52 | 37.59 | 12.16 | 309.10 | 0.2713 | 802.0 | 633.0 | |
| 0.00 | 0.85 | 0.00 | 0.44 | 5.61 | 37.05 | 11.61 | 310.63 | 0.2651 | 827.0 | 757.4 | |
| 0.00 | 1.02 | 0.00 | 0.52 | 6.36 | 32.11 | 6.67 | 328.15 | 0.2198 | 908.0 | 782.0 | |
| 0.00 | 1.02 | 0.00 | 0.51 | 0.46 | 30.72 | 5.29 | 312.35 | 0.1253 | 767.0 | 602.6 | |
| 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. | |