| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.39 | 42.34 | 2.71 | 21.35 | 14.52 | 261.23 | -7.65 | 43.98 | 0.1862 | 178.2 | 118.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.15 | 0.00 | 0.58 | 13.33 | 263.67 | -5.20 | 38.45 | 0.1426 | -777.0 | -529.3 | |
| 0.00 | 1.50 | 0.00 | 0.75 | 14.87 | 263.45 | -5.43 | 33.53 | 0.1662 | -953.0 | -738.3 | |
| 0.62 | 2.65 | 0.31 | 1.33 | 14.57 | 263.30 | -5.57 | 35.32 | 0.1634 | -1110.1 | -879.4 | |
| 0.00 | 5.39 | 0.00 | 2.71 | 14.75 | 262.89 | -5.98 | 36.58 | 0.1700 | -973.0 | -826.3 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 15.37 | 261.68 | -7.19 | 39.42 | 0.1910 | -863.0 | -693.5 | |
| 4.77 | 10.34 | 2.40 | 5.19 | 13.31 | 261.65 | -7.22 | 47.73 | 0.1661 | 1091.5 | 815.5 | |
| 0.00 | 1.41 | 0.00 | 0.71 | 15.18 | 261.37 | -7.50 | 41.24 | 0.1920 | -739.0 | -394.6 | |
| 0.00 | 2.92 | 0.00 | 1.47 | 13.48 | 261.30 | -7.57 | 48.25 | 0.1725 | 310.0 | 208.9 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 13.93 | 261.10 | -7.77 | 47.04 | 0.1802 | -955.0 | -718.6 | |
| 0.00 | 1.86 | 0.00 | 0.94 | 14.98 | 260.34 | -8.53 | 45.54 | 0.2017 | 792.0 | 589.1 | |
| 0.00 | 2.92 | 0.00 | 1.48 | 15.31 | 259.73 | -9.14 | 46.31 | 0.2129 | 896.0 | 662.3 | |
| 0.00 | 2.92 | 0.00 | 1.48 | 15.58 | 259.69 | -9.19 | 45.50 | 0.2166 | 933.0 | 839.6 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 13.64 | 259.70 | -9.17 | 52.80 | 0.1953 | 841.0 | 607.2 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 13.88 | 259.54 | -9.34 | 52.30 | 0.2000 | 666.0 | 566.7 | |
| 0.00 | 1.15 | 0.00 | 0.58 | 15.36 | 259.41 | -9.46 | 47.07 | 0.2175 | 844.0 | 560.8 | |
| 0.00 | 0.88 | 0.00 | 0.45 | 16.49 | 259.30 | -9.58 | 43.71 | 0.2319 | 857.0 | 557.7 | |
| 0.00 | 1.41 | 0.00 | 0.72 | 16.54 | 259.10 | -9.77 | 44.09 | 0.2349 | 784.0 | 535.2 | |
| 0.00 | 1.50 | 0.00 | 0.77 | 16.83 | 258.00 | -10.87 | 46.19 | 0.2513 | 685.0 | 488.6 | |
| 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. | |