| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.36 | 443.59 | 37.66 | 244.83 | 11.40 | 274.18 | -19.65 | 48.56 | 0.4408 | -577.4 | -313.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.53 | 11.94 | 277.97 | -15.86 | 41.61 | 0.4045 | -745.0 | -563.7 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 12.78 | 277.12 | -16.72 | 41.71 | 0.4234 | 601.0 | 555.1 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 12.41 | 276.98 | -16.86 | 42.55 | 0.4205 | 968.0 | 841.9 | |
| 0.00 | 0.53 | 0.00 | 0.29 | 13.38 | 275.29 | -18.55 | 43.70 | 0.4497 | 631.0 | 458.3 | |
| 62.18 | 380.84 | 34.06 | 208.64 | 11.00 | 274.91 | -18.92 | 48.28 | 0.4283 | -1440.0 | -414.1 | |
| 0.00 | 1.41 | 0.00 | 0.79 | 14.85 | 274.38 | -19.46 | 42.83 | 0.4756 | -860.0 | -589.2 | |
| 0.00 | 2.38 | 0.00 | 1.33 | 13.74 | 274.35 | -19.49 | 44.57 | 0.4638 | -687.0 | -530.3 | |
| 0.62 | 1.41 | 0.35 | 0.79 | 12.69 | 272.62 | -21.21 | 48.65 | 0.4722 | -850.9 | -730.2 | |
| 0.00 | 1.94 | 0.00 | 1.09 | 12.47 | 272.48 | -21.36 | 49.19 | 0.4718 | -834.0 | -664.2 | |
| 0.00 | 1.50 | 0.00 | 0.85 | 14.04 | 272.30 | -21.54 | 46.94 | 0.4894 | -586.0 | -525.7 | |
| 0.00 | 1.06 | 0.00 | 0.59 | 12.29 | 272.36 | -21.48 | 49.65 | 0.4713 | -715.0 | -548.5 | |
| 0.00 | 0.88 | 0.00 | 0.50 | 12.86 | 272.21 | -21.63 | 48.91 | 0.4787 | -559.0 | -474.2 | |
| 0.00 | 1.06 | 0.00 | 0.60 | 14.18 | 272.02 | -21.82 | 47.10 | 0.4939 | -457.0 | -456.7 | |
| 0.00 | 1.24 | 0.00 | 0.70 | 13.01 | 271.80 | -22.04 | 49.21 | 0.4848 | -680.0 | -492.9 | |
| 0.00 | 2.38 | 0.00 | 1.33 | 9.44 | 271.55 | -22.28 | 55.65 | 0.4549 | -859.0 | -697.6 | |
| 0.00 | 1.06 | 0.00 | 0.61 | 14.29 | 270.12 | -23.71 | 49.28 | 0.5163 | 764.0 | 631.2 | |
| 0.00 | 1.85 | 0.00 | 1.08 | 15.33 | 269.83 | -24.01 | 48.08 | 0.5294 | 788.0 | 673.6 | |
| 0.00 | 0.97 | 0.00 | 0.55 | 12.29 | 270.09 | -23.74 | 52.45 | 0.4982 | 732.0 | 542.9 | |
| 0.00 | 1.59 | 0.00 | 0.93 | 15.18 | 269.65 | -24.19 | 48.52 | 0.5300 | 822.0 | 746.3 | |
| 0.44 | 2.03 | 0.26 | 1.20 | 16.85 | 269.05 | -24.79 | 46.83 | 0.5523 | -901.6 | -718.6 | |
| 0.00 | 1.94 | 0.00 | 1.12 | 13.37 | 269.31 | -24.53 | 51.64 | 0.5172 | 816.0 | 604.1 | |
| 0.62 | 1.94 | 0.37 | 1.16 | 16.94 | 268.62 | -25.22 | 47.19 | 0.5577 | -760.6 | -568.0 | |
| 0.00 | 5.21 | 0.00 | 3.01 | 13.10 | 269.00 | -24.84 | 52.41 | 0.5184 | 612.0 | 777.3 | |
| 3.97 | 9.19 | 2.31 | 5.33 | 13.42 | 268.82 | -25.01 | 52.09 | 0.5233 | 888.0 | 578.3 | |
| 0.00 | 1.85 | 0.00 | 1.12 | 17.89 | 267.85 | -25.99 | 46.76 | 0.5747 | 710.0 | 593.6 | |
| 0.00 | 0.53 | 0.00 | 0.31 | 15.83 | 268.11 | -25.72 | 49.30 | 0.5529 | 643.0 | 531.7 | |
| 0.00 | 2.38 | 0.00 | 1.41 | 15.15 | 268.10 | -25.74 | 50.29 | 0.5470 | 859.0 | 698.8 | |
| 0.00 | 0.26 | 0.00 | 0.16 | 15.73 | 267.99 | -25.85 | 49.57 | 0.5535 | 616.0 | 619.7 | |
| 0.00 | 2.03 | 0.00 | 1.20 | 14.05 | 267.58 | -26.25 | 52.46 | 0.5433 | 966.0 | 757.9 | |
| 0.00 | 0.88 | 0.00 | 0.53 | 16.29 | 267.18 | -26.66 | 49.64 | 0.5674 | 476.0 | 414.8 | |
| 0.00 | 0.97 | 0.00 | 0.57 | 14.07 | 267.27 | -26.57 | 52.76 | 0.5471 | 548.0 | 432.2 | |
| 0.00 | 1.24 | 0.00 | 0.72 | 11.94 | 267.41 | -26.43 | 55.92 | 0.5278 | -353.0 | -347.4 | |
| 0.00 | 1.06 | 0.00 | 0.62 | 13.60 | 267.19 | -26.65 | 53.56 | 0.5440 | 831.0 | 703.9 | |
| 0.53 | 1.32 | 0.31 | 0.76 | 10.09 | 267.42 | -26.42 | 58.96 | 0.5133 | 809.5 | 679.9 | |
| 0.00 | 1.77 | 0.00 | 1.04 | 13.54 | 266.99 | -26.85 | 53.85 | 0.5460 | 815.0 | 706.5 | |
| 0.00 | 2.03 | 0.00 | 1.20 | 13.74 | 266.89 | -26.94 | 53.64 | 0.5487 | 748.0 | 610.9 | |
| 0.00 | 1.24 | 0.00 | 0.73 | 13.36 | 266.80 | -27.04 | 54.31 | 0.5467 | 697.0 | 498.1 | |
| 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. | |