| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.51 | 94.72 | 21.40 | 50.04 | -19.39 | 51.07 | 8.57 | 204.12 | 0.3479 | 413.5 | 358.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.26 | 53.78 | 13.36 | 28.44 | -19.08 | 52.56 | 10.06 | 208.13 | 0.3518 | 1084.9 | 719.3 | |
| 0.54 | -1.00 | 0.29 | -1.00 | -19.05 | 52.20 | 9.70 | 207.32 | 0.3486 | 1021.8 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -18.50 | 52.14 | 9.64 | 207.95 | 0.3403 | 840.0 | 636.2 | |
| 0.63 | -1.00 | 0.33 | -1.00 | -19.56 | 52.00 | 9.50 | 206.16 | 0.3545 | 708.3 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -18.31 | 51.87 | 9.37 | 207.56 | 0.3355 | 854.0 | 679.0 | |
| 0.00 | 1.71 | 0.00 | 0.90 | -18.47 | 51.84 | 9.35 | 207.27 | 0.3376 | 868.0 | 770.1 | |
| 0.00 | 1.26 | 0.00 | 0.67 | -19.27 | 51.66 | 9.16 | 205.72 | 0.3479 | 831.0 | 639.0 | |
| 0.00 | 1.99 | 0.00 | 1.04 | -17.24 | 51.42 | 8.93 | 208.05 | 0.3165 | 813.0 | 635.7 | |
| 0.00 | 1.71 | 0.00 | 0.89 | -16.98 | 50.51 | 8.02 | 205.97 | 0.3060 | 791.0 | 643.0 | |
| 0.00 | 0.90 | 0.00 | 0.48 | -20.36 | 50.61 | 8.11 | 201.84 | 0.3571 | 638.0 | 600.0 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -20.98 | 50.47 | 7.98 | 200.86 | 0.3656 | 771.0 | 633.7 | |
| 0.00 | 1.17 | 0.00 | 0.62 | -20.23 | 50.37 | 7.87 | 201.41 | 0.3538 | 425.0 | 447.3 | |
| 0.00 | 1.89 | 0.00 | 1.00 | -19.53 | 49.75 | 7.26 | 200.62 | 0.3394 | -886.0 | -645.2 | |
| 3.70 | 21.93 | 1.95 | 11.54 | -19.59 | 49.23 | 6.74 | 199.21 | 0.3375 | -1223.8 | -665.6 | |
| 10.38 | -14.00 | 5.47 | -14.00 | -19.85 | 49.21 | 6.72 | 198.89 | 0.3413 | -1042.4 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -23.45 | 48.61 | 6.12 | 194.41 | 0.3944 | 693.0 | 489.2 | |
| 0.00 | 3.70 | 0.00 | 1.97 | -22.31 | 41.98 | -0.51 | 178.69 | 0.3634 | -667.0 | -604.4 | |
| 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. | |