| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.72 | 41.95 | 5.96 | 32.58 | 7.76 | 252.08 | 50.47 | 276.93 | 0.7718 | 314.8 | 225.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.73 | 2.27 | 0.62 | 1.92 | 6.88 | 256.01 | 54.40 | 275.74 | 0.8135 | -445.6 | -327.4 | |
| 0.00 | 0.91 | 0.00 | 0.77 | 7.02 | 255.77 | 54.16 | 275.91 | 0.8111 | -350.0 | -344.2 | |
| 0.00 | 1.09 | 0.00 | 0.91 | 6.87 | 255.17 | 53.56 | 275.73 | 0.8049 | -388.0 | -443.3 | |
| 0.00 | 2.36 | 0.00 | 1.95 | 7.12 | 255.00 | 53.39 | 276.05 | 0.8032 | -704.0 | -610.4 | |
| 0.00 | 1.27 | 0.00 | 1.05 | 8.08 | 254.76 | 53.16 | 277.26 | 0.8009 | -672.0 | -622.2 | |
| 0.00 | 4.00 | 0.00 | 3.07 | 8.96 | 251.59 | 49.98 | 278.51 | 0.7672 | 589.0 | 495.1 | |
| 3.09 | 8.35 | 2.35 | 6.37 | 7.25 | 251.25 | 49.64 | 276.29 | 0.7627 | 684.2 | 450.7 | |
| 2.81 | 13.89 | 2.16 | 10.64 | 8.38 | 251.44 | 49.83 | 277.76 | 0.7652 | 572.9 | 351.5 | |
| 1.09 | -7.00 | 0.83 | -7.00 | 7.04 | 251.22 | 49.61 | 276.01 | 0.7623 | 567.2 | 999999 | |
| 0.00 | 0.73 | 0.00 | 0.56 | 9.36 | 251.57 | 49.96 | 279.03 | 0.7672 | 574.0 | 508.5 | |
| 0.00 | 0.45 | 0.00 | 0.34 | 5.86 | 250.92 | 49.31 | 274.46 | 0.7588 | 430.0 | 377.4 | |
| 0.00 | 1.36 | 0.00 | 1.04 | 8.82 | 251.23 | 49.62 | 278.35 | 0.7631 | 536.0 | 537.1 | |
| 0.00 | 1.27 | 0.00 | 0.97 | 8.47 | 250.97 | 49.36 | 277.90 | 0.7600 | 607.0 | 506.9 | |
| 0.00 | 1.00 | 0.00 | 0.75 | 5.86 | 250.40 | 48.79 | 274.45 | 0.7529 | 594.0 | 504.5 | |
| 0.00 | 1.45 | 0.00 | 1.09 | 6.16 | 250.39 | 48.78 | 274.86 | 0.7528 | 679.0 | 549.6 | |
| 0.00 | 0.82 | 0.00 | 0.61 | 6.48 | 250.15 | 48.54 | 275.29 | 0.7501 | 492.0 | 424.9 | |
| 0.00 | 0.73 | 0.00 | 0.54 | 6.12 | 250.11 | 48.50 | 274.80 | 0.7495 | 541.0 | 540.6 | |
| 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. | |