| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 85 | 573 | 45 | 306 | 2.29 | 271.54 | 21.34 | 266.16 | 0.3657 | 1631.4 | 637.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43 | 464 | 23 | 248 | 2.05 | 273.12 | 22.91 | 266.06 | 0.3917 | 1690.4 | 732.2 | |
| 8 | -1 | 4 | -1 | 2.18 | 272.41 | 22.21 | 266.25 | 0.3801 | 1598.6 | 999999 | |
| 0 | 20 | 0 | 11 | 3.92 | 272.33 | 22.12 | 270.83 | 0.3773 | 1121.0 | 789.0 | |
| 24 | -1 | 13 | -1 | 2.76 | 272.22 | 22.01 | 267.75 | 0.3762 | 1873.1 | 999999 | |
| 10 | -1 | 5 | -1 | 2.00 | 271.99 | 21.79 | 265.66 | 0.3736 | 1402.3 | 999999 | |
| 0 | 9 | 0 | 5 | 1.43 | 271.66 | 21.45 | 264.03 | 0.3692 | 1159.0 | 822.2 | |
| 0 | 9 | 0 | 5 | 4.35 | 271.67 | 21.47 | 272.01 | 0.3667 | 491.0 | 452.6 | |
| 0 | 3 | 0 | 2 | 0.13 | 271.11 | 20.91 | 260.29 | 0.3636 | 620.0 | 478.7 | |
| 0 | 4 | 0 | 2 | 0.94 | 269.76 | 19.55 | 261.90 | 0.3396 | 760.0 | 577.7 | |
| 0 | 5 | 0 | 2 | 2.48 | 265.86 | 15.65 | 265.31 | 0.2717 | 864.0 | 821.7 | |
| 0 | 3 | 0 | 2 | 1.08 | 264.45 | 14.25 | 259.20 | 0.2516 | 608.0 | 529.1 | |
| 0 | 5 | 0 | 3 | 0.32 | 263.62 | 13.41 | 255.41 | 0.2408 | 772.0 | 635.2 | |
| 0 | 3 | 0 | 2 | 2.26 | 263.04 | 12.83 | 263.11 | 0.2245 | -659.0 | -739.8 | |
| 0 | 4 | 0 | 2 | 4.57 | 262.87 | 12.66 | 273.53 | 0.2199 | -669.0 | -551.1 | |
| 0 | 7 | 0 | 3 | 1.11 | 262.71 | 12.51 | 257.77 | 0.2225 | 348.0 | 356.9 | |
| 0 | 10 | 0 | 5 | 0.77 | 262.36 | 12.15 | 255.87 | 0.2180 | 698.0 | 591.7 | |
| 0 | 27 | 0 | 14 | 2.65 | 262.33 | 12.12 | 264.53 | 0.2117 | -1005.0 | -700.0 | |
| 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. | |