| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.90 | 391.52 | 34.21 | 215.90 | 15.01 | 133.62 | 25.05 | 291.00 | 0.4399 | -892.9 | -373.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.56 | 17.08 | 135.39 | 26.81 | 294.28 | 0.4750 | 495.0 | 423.9 | |
| 60.91 | 366.92 | 33.70 | 202.92 | 15.20 | 134.02 | 25.45 | 291.23 | 0.4467 | -1475.6 | -433.0 | |
| 0.00 | 1.80 | 0.00 | 0.99 | 13.70 | 133.22 | 24.64 | 288.38 | 0.4287 | -703.0 | -480.8 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 15.90 | 132.90 | 24.32 | 293.50 | 0.4338 | -836.0 | -662.8 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 16.51 | 131.80 | 23.23 | 295.68 | 0.4213 | -880.0 | -759.7 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 12.57 | 127.33 | 18.76 | 289.45 | 0.3343 | 752.0 | 573.3 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 12.78 | 127.34 | 18.77 | 290.05 | 0.3355 | 774.0 | 583.2 | |
| 0.00 | 1.35 | 0.00 | 0.71 | 12.49 | 127.03 | 18.45 | 289.47 | 0.3292 | 818.0 | 685.9 | |
| 0.00 | 2.08 | 0.00 | 1.09 | 12.34 | 126.88 | 18.31 | 289.15 | 0.3263 | 950.0 | 736.5 | |
| 0.00 | 1.17 | 0.00 | 0.61 | 12.43 | 126.20 | 17.63 | 290.00 | 0.3161 | 672.0 | 501.8 | |
| 0.00 | 1.44 | 0.00 | 0.75 | 9.97 | 125.66 | 17.09 | 282.61 | 0.2978 | 734.0 | 568.4 | |
| 0.00 | 3.25 | 0.00 | 1.69 | 10.25 | 125.64 | 17.07 | 283.53 | 0.2984 | 635.0 | 655.6 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 6.77 | 125.09 | 16.52 | 271.73 | 0.2838 | 843.0 | 642.8 | |
| 0.00 | 1.35 | 0.00 | 0.70 | 10.82 | 125.06 | 16.49 | 285.83 | 0.2910 | 1045.0 | 891.3 | |
| 0.00 | 1.26 | 0.00 | 0.66 | 14.16 | 124.73 | 16.16 | 296.89 | 0.3039 | 780.0 | 597.5 | |
| 0.99 | 3.70 | 0.51 | 1.91 | 10.30 | 124.23 | 15.66 | 284.68 | 0.2757 | 1179.9 | 905.2 | |
| 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. | |