| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.96 | 89.37 | 22.59 | 68.50 | 19.84 | 64.41 | 42.69 | 303.39 | 0.7654 | 190.8 | 316.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.83 | 0.00 | 2.35 | 19.32 | 69.09 | 47.37 | 300.23 | 0.8058 | 183.0 | 116.3 | |
| 12.17 | 17.82 | 10.02 | 14.69 | 19.25 | 68.65 | 46.92 | 300.37 | 0.8015 | -608.0 | -303.6 | |
| 0.00 | 0.86 | 0.00 | 0.71 | 19.68 | 68.40 | 46.67 | 300.98 | 0.8012 | -321.0 | -281.2 | |
| 0.00 | 0.86 | 0.00 | 0.70 | 18.97 | 68.04 | 46.31 | 300.35 | 0.7947 | -607.0 | -543.0 | |
| 0.00 | 0.86 | 0.00 | 0.67 | 19.03 | 65.83 | 44.11 | 301.58 | 0.7746 | 294.0 | 214.0 | |
| 0.00 | 1.20 | 0.00 | 0.93 | 19.18 | 65.71 | 43.98 | 301.83 | 0.7742 | 426.0 | 377.9 | |
| 0.00 | 1.03 | 0.00 | 0.79 | 18.90 | 65.39 | 43.67 | 301.67 | 0.7698 | 406.0 | 412.5 | |
| 0.00 | 1.54 | 0.00 | 1.19 | 18.69 | 65.28 | 43.56 | 301.49 | 0.7678 | 569.0 | 431.3 | |
| 0.00 | 1.11 | 0.00 | 0.84 | 19.38 | 63.79 | 42.06 | 303.15 | 0.7572 | 661.0 | 522.9 | |
| 0.00 | 2.31 | 0.00 | 1.76 | 20.32 | 63.67 | 41.95 | 304.31 | 0.7612 | 468.0 | 355.4 | |
| 0.00 | 1.20 | 0.00 | 0.91 | 19.98 | 63.52 | 41.79 | 304.01 | 0.7579 | 585.0 | 473.3 | |
| 1.54 | 1.97 | 1.19 | 1.52 | 21.91 | 63.67 | 41.95 | 306.12 | 0.7701 | -441.3 | -406.4 | |
| 5.57 | 52.09 | 4.15 | 38.79 | 19.82 | 62.75 | 41.02 | 304.28 | 0.7497 | 839.6 | 442.6 | |
| 9.68 | -13.00 | 7.23 | -13.00 | 20.17 | 62.65 | 40.93 | 304.75 | 0.7508 | 686.5 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.19 | 23.34 | 61.05 | 39.32 | 309.40 | 0.7553 | 514.0 | 437.0 | |
| 0.00 | 1.46 | 0.00 | 1.05 | 20.59 | 60.11 | 38.38 | 306.90 | 0.7292 | 659.0 | 570.7 | |
| 0.00 | 0.77 | 0.00 | 0.55 | 20.39 | 60.05 | 38.32 | 306.71 | 0.7273 | 632.0 | 525.6 | |
| 0.00 | 1.20 | 0.00 | 0.86 | 20.55 | 59.61 | 37.89 | 307.20 | 0.7242 | 683.0 | 538.4 | |
| 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. | |