| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.14 | 283.02 | 35.16 | 210.92 | 12.82 | 13.22 | 44.73 | 293.15 | 0.7486 | -784.7 | -295.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.59 | 0.00 | 1.19 | 10.67 | 14.38 | 45.89 | 289.93 | 0.7528 | -728.0 | -654.4 | |
| 0.00 | 0.88 | 0.00 | 0.66 | 10.58 | 14.05 | 45.56 | 289.95 | 0.7490 | -720.0 | -608.0 | |
| 42.38 | 268.38 | 31.63 | 200.41 | 12.79 | 13.38 | 44.89 | 293.03 | 0.7502 | -1129.0 | -305.1 | |
| 4.76 | -3.00 | 3.53 | -3.00 | 13.37 | 12.78 | 44.29 | 294.04 | 0.7462 | -788.5 | 999999 | |
| 0.00 | 1.50 | 0.00 | 1.08 | 12.30 | 11.86 | 43.37 | 293.11 | 0.7317 | -633.0 | -542.2 | |
| 0.00 | 0.79 | 0.00 | 0.59 | 15.05 | 12.20 | 43.71 | 296.41 | 0.7474 | 383.0 | 381.4 | |
| 0.00 | 1.06 | 0.00 | 0.76 | 12.72 | 11.61 | 43.12 | 293.77 | 0.7308 | -760.0 | -589.2 | |
| 0.00 | 0.88 | 0.00 | 0.64 | 12.99 | 11.50 | 43.01 | 294.17 | 0.7308 | -190.0 | -234.3 | |
| 0.00 | 1.06 | 0.00 | 0.76 | 12.03 | 11.25 | 42.76 | 293.05 | 0.7240 | -489.0 | -440.0 | |
| 0.00 | 1.06 | 0.00 | 0.77 | 13.53 | 11.53 | 43.04 | 294.84 | 0.7336 | -421.0 | -370.0 | |
| 0.00 | 0.97 | 0.00 | 0.70 | 13.04 | 11.21 | 42.72 | 294.37 | 0.7279 | -526.0 | -453.4 | |
| 0.00 | 0.79 | 0.00 | 0.56 | 11.56 | 10.74 | 42.25 | 292.67 | 0.7163 | 509.0 | 343.0 | |
| 0.00 | 0.44 | 0.00 | 0.31 | 11.56 | 10.37 | 41.88 | 292.86 | 0.7121 | 453.0 | 393.2 | |
| 0.00 | 0.62 | 0.00 | 0.43 | 11.71 | 10.28 | 41.79 | 293.11 | 0.7117 | 478.0 | 471.6 | |
| 0.00 | 0.88 | 0.00 | 0.61 | 11.15 | 9.48 | 40.99 | 292.76 | 0.7002 | 481.0 | 437.1 | |
| 0.00 | 0.97 | 0.00 | 0.67 | 11.93 | 9.01 | 40.52 | 294.05 | 0.6984 | 668.0 | 491.6 | |
| 0.00 | 1.15 | 0.00 | 0.78 | 14.84 | 7.02 | 38.53 | 299.02 | 0.6909 | 625.0 | 548.8 | |
| 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. | |