| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.96 | 71.01 | 10.73 | 36.30 | 6.62 | 10.72 | 3.30 | 346.64 | 0.2480 | 72.2 | 191.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.73 | 2.86 | 0.89 | 1.47 | 5.89 | 14.16 | 6.74 | 332.69 | 0.2555 | -1052.8 | -968.2 | |
| 0.00 | 1.13 | 0.00 | 0.58 | 6.10 | 13.86 | 6.44 | 334.10 | 0.2565 | -976.0 | -868.3 | |
| 0.00 | 2.69 | 0.00 | 1.38 | 6.65 | 13.36 | 5.93 | 336.75 | 0.2614 | -1154.0 | -879.2 | |
| 0.00 | 2.60 | 0.00 | 1.33 | 6.03 | 13.23 | 5.81 | 336.25 | 0.2509 | -1031.0 | -715.8 | |
| 7.54 | 10.75 | 3.87 | 5.51 | 7.25 | 11.71 | 4.29 | 343.45 | 0.2614 | -945.0 | -640.0 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 6.78 | 10.77 | 3.35 | 346.50 | 0.2497 | 866.0 | 637.2 | |
| 0.69 | 1.73 | 0.35 | 0.88 | 5.31 | 10.61 | 3.19 | 345.66 | 0.2247 | 1069.6 | 914.6 | |
| 0.00 | 1.13 | 0.00 | 0.57 | 5.06 | 10.58 | 3.16 | 345.53 | 0.2206 | 921.0 | 722.9 | |
| 0.00 | 1.30 | 0.00 | 0.66 | 6.84 | 10.59 | 3.17 | 347.25 | 0.2500 | 583.0 | 386.3 | |
| 0.35 | 3.29 | 0.18 | 1.68 | 5.55 | 10.34 | 2.92 | 347.07 | 0.2277 | 957.8 | 778.1 | |
| 2.51 | 15.78 | 1.29 | 8.09 | 7.48 | 10.12 | 2.69 | 349.59 | 0.2591 | -848.3 | 6.3 | |
| 4.07 | 13.61 | 2.07 | 6.93 | 5.88 | 9.84 | 2.41 | 349.52 | 0.2315 | 1030.9 | 637.6 | |
| 4.07 | 10.06 | 2.08 | 5.14 | 6.80 | 9.72 | 2.30 | 350.66 | 0.2466 | 1068.9 | 719.7 | |
| 0.00 | 2.17 | 0.00 | 1.10 | 6.25 | 8.70 | 1.28 | 354.56 | 0.2350 | 973.0 | 804.1 | |
| 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. | |