| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 91.42 | 463.22 | 66.42 | 337.84 | 18.54 | 166.25 | -41.20 | 58.39 | 0.7340 | -326.3 | -181.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.27 | 353.27 | 0.19 | 249.54 | 18.23 | 168.84 | -38.61 | 57.31 | 0.7065 | -1113.3 | -334.9 | |
| 11.87 | -1.00 | 8.31 | -1.00 | 18.05 | 168.56 | -38.89 | 57.71 | 0.7084 | -1151.9 | 999999 | |
| 28.97 | -1.00 | 20.45 | -1.00 | 18.69 | 168.31 | -39.14 | 57.08 | 0.7147 | -989.9 | 999999 | |
| 26.49 | -1.00 | 18.76 | -1.00 | 18.32 | 167.87 | -39.58 | 57.80 | 0.7170 | -906.6 | 999999 | |
| 2.39 | -1.00 | 1.71 | -1.00 | 18.89 | 167.72 | -39.73 | 57.20 | 0.7219 | -537.7 | 999999 | |
| 4.07 | -1.00 | 2.91 | -1.00 | 18.46 | 167.30 | -40.15 | 57.98 | 0.7237 | -513.2 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.66 | 20.32 | 165.88 | -41.57 | 56.56 | 0.7480 | -499.0 | -427.5 | |
| 0.00 | 0.97 | 0.00 | 0.71 | 18.48 | 166.37 | -41.08 | 58.50 | 0.7333 | -158.0 | -162.5 | |
| 0.00 | 0.89 | 0.00 | 0.65 | 18.40 | 166.05 | -41.40 | 58.77 | 0.7361 | -231.0 | -181.3 | |
| 0.00 | 0.62 | 0.00 | 0.46 | 19.11 | 165.75 | -41.70 | 58.09 | 0.7428 | 239.0 | 287.4 | |
| 0.00 | 0.53 | 0.00 | 0.39 | 17.82 | 165.45 | -42.00 | 59.82 | 0.7391 | -440.0 | -321.0 | |
| 0.00 | 1.95 | 0.00 | 1.49 | 19.58 | 163.68 | -43.77 | 58.67 | 0.7653 | 632.0 | 461.7 | |
| 0.00 | 0.97 | 0.00 | 0.76 | 19.72 | 163.05 | -44.40 | 58.83 | 0.7720 | 473.0 | 433.5 | |
| 0.00 | 1.86 | 0.00 | 1.45 | 19.50 | 162.86 | -44.59 | 59.19 | 0.7728 | 610.0 | 526.3 | |
| 0.00 | 1.95 | 0.00 | 1.49 | 17.63 | 163.08 | -44.37 | 61.31 | 0.7621 | 558.0 | 511.9 | |
| 0.00 | 0.27 | 0.00 | 0.21 | 19.43 | 162.48 | -44.97 | 59.47 | 0.7761 | 497.0 | 541.3 | |
| 0.00 | 0.62 | 0.00 | 0.49 | 19.33 | 162.10 | -45.35 | 59.78 | 0.7791 | 475.0 | 442.0 | |
| 0.00 | 3.19 | 0.00 | 2.45 | 17.27 | 162.56 | -44.89 | 61.99 | 0.7656 | 815.0 | 676.7 | |
| 0.00 | 0.89 | 0.00 | 0.68 | 17.67 | 162.44 | -45.01 | 61.58 | 0.7685 | 527.0 | 484.7 | |
| 0.00 | 0.53 | 0.00 | 0.42 | 19.17 | 161.93 | -45.52 | 60.04 | 0.7801 | 482.0 | 512.3 | |
| 0.00 | 0.97 | 0.00 | 0.77 | 19.52 | 161.72 | -45.73 | 59.75 | 0.7837 | 504.0 | 429.1 | |
| 0.00 | 2.48 | 0.00 | 1.99 | 20.23 | 161.40 | -46.05 | 59.07 | 0.7897 | 474.0 | 389.6 | |
| 0.00 | 1.24 | 0.00 | 0.99 | 19.79 | 161.57 | -45.88 | 59.50 | 0.7862 | 563.0 | 498.6 | |
| 0.00 | 0.27 | 0.00 | 0.21 | 19.36 | 161.68 | -45.77 | 59.95 | 0.7832 | 424.0 | 405.7 | |
| 0.00 | 0.89 | 0.00 | 0.70 | 18.72 | 161.86 | -45.59 | 60.61 | 0.7787 | 483.0 | 424.7 | |
| 0.00 | 1.15 | 0.00 | 0.88 | 16.67 | 162.43 | -45.02 | 62.79 | 0.7642 | 530.0 | 540.6 | |
| 0.00 | 1.33 | 0.00 | 1.02 | 17.04 | 162.19 | -45.26 | 62.46 | 0.7683 | 505.0 | 393.3 | |
| 0.00 | 1.42 | 0.00 | 1.11 | 17.91 | 161.77 | -45.68 | 61.61 | 0.7761 | 647.0 | 539.7 | |
| 0.00 | 2.30 | 0.00 | 1.82 | 18.58 | 161.54 | -45.91 | 60.93 | 0.7811 | 497.0 | 428.0 | |
| 0.00 | 1.86 | 0.00 | 1.45 | 17.52 | 161.81 | -45.64 | 62.06 | 0.7740 | 633.0 | 488.2 | |
| 0.00 | 1.42 | 0.00 | 1.11 | 17.59 | 161.69 | -45.76 | 62.03 | 0.7755 | 384.0 | 362.9 | |
| 8.77 | 78.49 | 7.10 | 63.94 | 18.95 | 160.44 | -47.01 | 61.02 | 0.7931 | 864.8 | 137.9 | |
| 1.95 | -32.00 | 1.59 | -32.00 | 19.33 | 160.25 | -47.20 | 60.67 | 0.7964 | 542.7 | 999999 | |
| 2.39 | -32.00 | 1.94 | -32.00 | 18.73 | 160.33 | -47.12 | 61.32 | 0.7932 | 860.6 | 999999 | |
| 4.25 | -32.00 | 3.46 | -32.00 | 18.66 | 160.03 | -47.42 | 61.55 | 0.7957 | 609.5 | 999999 | |
| 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. | |