| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.18 | 275.41 | 23.54 | 144.07 | 12.31 | 262.81 | -4.07 | 12.08 | 0.3204 | -748.3 | -383.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.33 | 0.00 | 0.69 | 12.84 | 265.71 | -1.18 | 3.62 | 0.3193 | 782.0 | 630.3 | |
| 5.04 | 257.02 | 2.63 | 133.94 | 12.34 | 263.77 | -3.12 | 9.75 | 0.3149 | -1253.1 | -438.1 | |
| 17.86 | -2.00 | 9.30 | -2.00 | 12.06 | 263.74 | -3.14 | 10.00 | 0.3103 | -1562.9 | 999999 | |
| 22.28 | -2.00 | 11.61 | -2.00 | 12.09 | 263.34 | -3.55 | 11.22 | 0.3121 | -1387.6 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.77 | 18.71 | 262.66 | -4.23 | 9.60 | 0.4200 | -806.0 | -682.0 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 18.27 | 258.62 | -8.26 | 18.64 | 0.4288 | -719.0 | -562.1 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 18.08 | 258.28 | -8.60 | 19.51 | 0.4277 | -749.0 | -591.7 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 14.82 | 256.85 | -10.04 | 25.81 | 0.3888 | 688.0 | 470.4 | |
| 0.00 | 1.59 | 0.00 | 0.88 | 18.06 | 255.68 | -11.21 | 24.76 | 0.4429 | -867.0 | -692.0 | |
| 0.00 | 0.88 | 0.00 | 0.49 | 17.16 | 254.93 | -11.95 | 27.15 | 0.4354 | 874.0 | 714.7 | |
| 0.00 | 1.06 | 0.00 | 0.58 | 16.05 | 253.98 | -12.91 | 30.30 | 0.4274 | 790.0 | 627.9 | |
| 0.00 | 1.33 | 0.00 | 0.72 | 13.25 | 253.16 | -13.73 | 35.72 | 0.3974 | 591.0 | 516.2 | |
| 0.00 | 1.24 | 0.00 | 0.69 | 15.62 | 250.61 | -16.27 | 36.92 | 0.4511 | 792.0 | 582.2 | |
| 0.00 | 1.06 | 0.00 | 0.59 | 16.14 | 249.59 | -17.29 | 37.88 | 0.4670 | 794.0 | 587.0 | |
| 0.00 | 1.59 | 0.00 | 0.89 | 11.64 | 245.17 | -21.71 | 51.27 | 0.4663 | 735.0 | 565.3 | |
| 0.00 | 1.06 | 0.00 | 0.60 | 11.01 | 243.73 | -23.15 | 54.14 | 0.4782 | 817.0 | 710.7 | |
| 0.00 | 1.24 | 0.00 | 0.70 | 11.11 | 243.52 | -23.36 | 54.20 | 0.4817 | 793.0 | 580.4 | |
| 0.00 | 1.06 | 0.00 | 0.60 | 11.21 | 243.45 | -23.44 | 54.12 | 0.4835 | 585.0 | 500.5 | |
| 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. | |