| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61 | 544 | 34 | 298 | -29.34 | 22.02 | 8.41 | 197.57 | 0.4263 | -1652.1 | -395.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | -26.38 | 23.41 | 9.79 | 203.20 | 0.3884 | 528.0 | 425.0 | |
| 61 | 427 | 34 | 234 | -28.99 | 23.51 | 9.90 | 200.72 | 0.4269 | -1925.0 | -689.1 | |
| -2 | -2 | -2 | -2 | -29.21 | 22.91 | 9.30 | 199.38 | 0.4269 | 999999 | 999999 | |
| 0 | 5 | 0 | 3 | -29.36 | 21.23 | 7.62 | 196.01 | 0.4210 | -618.0 | -451.0 | |
| 0 | 5 | 0 | 3 | -29.57 | 20.41 | 6.80 | 194.21 | 0.4209 | 816.0 | 732.7 | |
| 0 | 9 | 0 | 5 | -30.04 | 20.31 | 6.69 | 193.71 | 0.4276 | 862.0 | 700.1 | |
| 0 | 2 | 0 | 1 | -30.08 | 19.95 | 6.34 | 192.99 | 0.4270 | 631.0 | 495.9 | |
| 0 | 12 | 0 | 6 | -29.63 | 19.21 | 5.60 | 191.78 | 0.4175 | 1038.0 | 743.5 | |
| 0 | 3 | 0 | 2 | -30.14 | 18.80 | 5.19 | 190.67 | 0.4241 | 604.0 | 474.9 | |
| 0 | 4 | 0 | 2 | -31.54 | 18.42 | 4.81 | 189.29 | 0.4448 | 800.0 | 628.9 | |
| 0 | 4 | 0 | 2 | -30.39 | 18.32 | 4.71 | 189.59 | 0.4268 | 626.0 | 555.7 | |
| 0 | 7 | 0 | 4 | -30.57 | 17.13 | 3.51 | 187.13 | 0.4268 | 1142.0 | 897.1 | |
| 0 | 3 | 0 | 2 | -30.83 | 16.91 | 3.30 | 186.62 | 0.4304 | 898.0 | 780.1 | |
| 0 | 9 | 0 | 5 | -30.11 | 16.84 | 3.23 | 186.71 | 0.4190 | 1000.0 | 802.2 | |
| 0 | 9 | 0 | 5 | -30.32 | 16.58 | 2.97 | 186.11 | 0.4219 | 861.0 | 737.5 | |
| 0 | 7 | 0 | 4 | -30.91 | 16.07 | 2.45 | 184.91 | 0.4305 | 815.0 | 696.8 | |
| 0 | 4 | 0 | 2 | -30.70 | 15.84 | 2.22 | 184.50 | 0.4268 | 902.0 | 655.2 | |
| 0 | 4 | 0 | 2 | -31.04 | 15.53 | 1.92 | 183.83 | 0.4319 | 810.0 | 760.5 | |
| 0 | 5 | 0 | 3 | -30.96 | 15.17 | 1.56 | 183.12 | 0.4302 | 1206.0 | 936.5 | |
| 0 | 13 | 0 | 7 | -30.96 | 14.77 | 1.16 | 182.32 | 0.4299 | 1058.0 | 811.8 | |
| 0 | 6 | 0 | 3 | -30.96 | 14.37 | 0.76 | 181.51 | 0.4297 | 1021.0 | 876.6 | |
| 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. | |