| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73 | 372 | 63 | 310 | 16.76 | 307.71 | 53.68 | 287.37 | 0.8095 | 86.8 | 209.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 6 | 17.29 | 316.84 | 62.81 | 287.03 | 0.8901 | -182.0 | -294.0 | |
| 8 | 45 | 8 | 41 | 14.99 | 311.12 | 57.09 | 284.81 | 0.8409 | -445.7 | -53.1 | |
| 8 | 25 | 7 | 23 | 16.47 | 310.93 | 56.90 | 286.59 | 0.8403 | 127.9 | 289.6 | |
| 2 | 9 | 1 | 8 | 14.54 | 310.04 | 56.01 | 284.36 | 0.8306 | -338.1 | -291.7 | |
| 0 | 4 | 0 | 4 | 17.08 | 310.99 | 56.95 | 287.31 | 0.8413 | 633.0 | 518.2 | |
| 0 | 12 | 0 | 10 | 16.94 | 310.02 | 55.98 | 287.25 | 0.8324 | 845.0 | 686.4 | |
| 3 | 12 | 3 | 11 | 17.95 | 309.67 | 55.64 | 288.50 | 0.8302 | 334.5 | 236.1 | |
| 0 | 10 | 0 | 8 | 14.42 | 308.13 | 54.10 | 284.39 | 0.8121 | -553.0 | -472.7 | |
| 2 | 17 | 2 | 14 | 14.66 | 307.66 | 53.62 | 284.72 | 0.8076 | -796.1 | -718.2 | |
| 4 | -9 | 4 | -9 | 15.02 | 307.65 | 53.62 | 285.18 | 0.8078 | -641.3 | 999999 | |
| 9 | 52 | 8 | 44 | 17.62 | 308.49 | 54.46 | 288.26 | 0.8188 | 736.3 | 563.2 | |
| 9 | -11 | 8 | -11 | 17.28 | 308.06 | 54.02 | 287.90 | 0.8142 | 841.5 | 999999 | |
| 0 | 3 | 0 | 2 | 16.53 | 307.60 | 53.57 | 287.05 | 0.8090 | 600.0 | 567.7 | |
| 0 | 6 | 0 | 5 | 15.85 | 306.72 | 52.69 | 286.32 | 0.7994 | -196.0 | -313.5 | |
| 7 | 95 | 6 | 77 | 17.94 | 306.12 | 52.08 | 289.01 | 0.7961 | 813.7 | 577.7 | |
| 0 | 6 | 0 | 4 | 15.92 | 305.07 | 51.03 | 286.63 | 0.7826 | -441.0 | -474.8 | |
| 6 | 24 | 5 | 19 | 17.16 | 305.40 | 51.36 | 288.16 | 0.7877 | 787.5 | 472.6 | |
| 0 | 5 | 0 | 4 | 16.92 | 304.65 | 50.61 | 287.98 | 0.7796 | -572.0 | -419.5 | |
| 0 | 5 | 0 | 4 | 18.50 | 304.34 | 50.31 | 290.04 | 0.7790 | -257.0 | -52.5 | |
| 15 | 36 | 11 | 26 | 16.55 | 301.42 | 47.38 | 288.07 | 0.7443 | -875.4 | -272.4 | |
| 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. | |