| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.04 | 0.00 | 10.86 | 4.87 | 256.56 | 32.76 | 278.82 | 0.5387 | 248.9 | 191.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.95 | 4.78 | 272.50 | 48.69 | 275.89 | 0.7548 | -644.0 | -528.1 | |
| 0.00 | 1.00 | 0.00 | 0.73 | 5.44 | 271.00 | 47.20 | 276.90 | 0.7380 | -483.0 | -422.9 | |
| 0.00 | 1.18 | 0.00 | 0.85 | 5.23 | 270.22 | 46.41 | 276.70 | 0.7286 | -688.0 | -518.0 | |
| 0.00 | 0.27 | 0.00 | 0.19 | -0.13 | 269.08 | 45.28 | 269.28 | 0.7129 | -504.0 | -454.0 | |
| 0.00 | 1.27 | 0.00 | 0.89 | -0.28 | 268.78 | 44.98 | 269.06 | 0.7092 | -341.0 | -325.4 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 4.31 | 256.24 | 32.43 | 277.18 | 0.5411 | 728.0 | 558.1 | |
| 0.00 | 1.81 | 0.00 | 1.05 | 9.32 | 254.20 | 30.39 | 287.14 | 0.5245 | 748.0 | 566.0 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 6.77 | 253.84 | 30.04 | 282.46 | 0.5111 | 596.0 | 449.8 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 6.56 | 253.62 | 29.81 | 282.13 | 0.5072 | 663.0 | 507.6 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 7.08 | 253.65 | 29.85 | 283.13 | 0.5092 | 594.0 | 458.5 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 4.32 | 248.57 | 24.77 | 279.10 | 0.4249 | 794.0 | 663.2 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 4.14 | 248.20 | 24.39 | 278.80 | 0.4186 | 732.0 | 555.6 | |
| 0.00 | 2.26 | 0.00 | 1.22 | 6.75 | 246.01 | 22.20 | 286.19 | 0.3924 | 717.0 | 569.6 | |
| 0.00 | 2.26 | 0.00 | 1.17 | 1.43 | 239.98 | 16.17 | 273.31 | 0.2801 | 572.0 | 330.5 | |
| 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. | |