| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.42 | 297.43 | 48.15 | 288.87 | -19.20 | 253.92 | 55.61 | 244.97 | 0.8621 | 723.1 | 225.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.42 | 275.26 | 48.15 | 268.07 | -19.10 | 254.06 | 55.75 | 245.13 | 0.8630 | 897.7 | 233.8 | |
| 0.00 | 0.82 | 0.00 | 0.80 | -20.59 | 253.58 | 55.27 | 243.32 | 0.8630 | 422.0 | 292.6 | |
| 0.00 | 1.00 | 0.00 | 0.99 | -21.30 | 253.86 | 55.55 | 242.62 | 0.8672 | 426.0 | 383.3 | |
| 0.00 | 1.45 | 0.00 | 1.41 | -20.72 | 253.48 | 55.16 | 243.14 | 0.8626 | 389.0 | 321.6 | |
| 0.00 | 3.18 | 0.00 | 3.05 | -20.26 | 253.06 | 54.75 | 243.51 | 0.8580 | 192.0 | 174.1 | |
| 0.00 | 1.36 | 0.00 | 1.26 | -19.25 | 252.11 | 53.80 | 244.32 | 0.8474 | 299.0 | 288.6 | |
| 0.00 | 5.18 | 0.00 | 4.81 | -19.54 | 252.09 | 53.77 | 243.98 | 0.8480 | 697.0 | 551.4 | |
| 0.00 | 1.27 | 0.00 | 1.19 | -19.88 | 252.14 | 53.83 | 243.62 | 0.8494 | 493.0 | 462.8 | |
| 0.00 | 1.09 | 0.00 | 1.00 | -20.05 | 251.62 | 53.31 | 243.25 | 0.8456 | -125.0 | -60.7 | |
| 0.00 | 1.73 | 0.00 | 1.64 | -22.37 | 252.01 | 53.70 | 240.81 | 0.8558 | -95.0 | -135.3 | |
| 0.00 | 1.45 | 0.00 | 1.37 | -22.21 | 251.59 | 53.28 | 240.83 | 0.8519 | -248.0 | -302.6 | |
| 0.00 | 0.91 | 0.00 | 0.82 | -20.87 | 250.29 | 51.98 | 241.84 | 0.8370 | -551.0 | -456.3 | |
| 0.00 | 0.91 | 0.00 | 0.83 | -21.73 | 250.73 | 52.41 | 241.04 | 0.8434 | -239.0 | -270.1 | |
| 0.00 | 1.82 | 0.00 | 1.63 | -21.12 | 249.99 | 51.68 | 241.45 | 0.8353 | -667.0 | -558.9 | |
| 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. | |