| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.08 | 0.00 | 11.75 | 11.02 | 258.89 | 11.48 | 294.69 | 0.2266 | 648.4 | 626.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.72 | 0.00 | 0.39 | 14.22 | 269.71 | 22.30 | 292.50 | 0.3999 | -571.0 | -448.2 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 17.56 | 267.24 | 19.83 | 302.77 | 0.3862 | -823.0 | -622.2 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 6.88 | 260.06 | 12.65 | 275.22 | 0.2193 | 661.0 | 572.8 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 5.42 | 259.90 | 12.49 | 268.51 | 0.2163 | 736.0 | 601.2 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 9.35 | 260.02 | 12.61 | 286.27 | 0.2254 | 760.0 | 618.1 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 8.87 | 259.72 | 12.31 | 284.48 | 0.2185 | 813.0 | 656.2 | |
| 0.00 | 2.44 | 0.00 | 1.24 | 9.91 | 259.25 | 11.84 | 289.71 | 0.2157 | 841.0 | 745.8 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 10.25 | 259.14 | 11.73 | 291.37 | 0.2157 | 798.0 | 677.4 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 9.70 | 259.09 | 11.68 | 289.01 | 0.2119 | 974.0 | 815.1 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 9.50 | 258.67 | 11.26 | 288.65 | 0.2042 | 921.0 | 768.0 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 8.53 | 258.26 | 10.85 | 284.47 | 0.1931 | 623.0 | 429.9 | |
| 0.00 | 2.98 | 0.00 | 1.51 | 9.27 | 258.07 | 10.65 | 288.42 | 0.1932 | 891.0 | 819.2 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.79 | 258.22 | 10.81 | 313.92 | 0.2517 | 891.0 | 733.0 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 16.16 | 258.08 | 10.67 | 315.37 | 0.2543 | 920.0 | 750.7 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 15.95 | 258.04 | 10.63 | 314.86 | 0.2513 | 889.0 | 745.6 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 17.44 | 257.80 | 10.39 | 319.57 | 0.2665 | 871.0 | 706.2 | |
| 0.00 | 0.63 | 0.00 | 0.32 | 4.13 | 256.09 | 8.68 | 258.95 | 0.1541 | 524.0 | 481.4 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 15.29 | 248.01 | 0.60 | 356.45 | 0.1645 | 953.0 | 769.3 | |
| 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. | |