| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.22 | 0.00 | 15.20 | 13.48 | 58.20 | -43.52 | 76.81 | 0.6872 | -49.6 | 3.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.70 | 17.57 | 73.79 | -27.93 | 65.22 | 0.4938 | -742.0 | -627.3 | |
| 0.00 | 0.97 | 0.00 | 0.62 | 14.24 | 62.43 | -39.28 | 75.31 | 0.6368 | -584.0 | -465.5 | |
| 0.00 | 1.49 | 0.00 | 0.95 | 11.87 | 62.44 | -39.28 | 79.03 | 0.6333 | -644.0 | -562.4 | |
| 0.00 | 1.93 | 0.00 | 1.26 | 15.37 | 61.54 | -40.18 | 73.75 | 0.6503 | -330.0 | -331.5 | |
| 0.00 | 0.70 | 0.00 | 0.45 | 12.24 | 62.10 | -39.62 | 78.49 | 0.6383 | -589.0 | -535.4 | |
| 0.00 | 1.23 | 0.00 | 0.79 | 12.83 | 61.87 | -39.85 | 77.60 | 0.6420 | -405.0 | -324.2 | |
| 0.00 | 0.88 | 0.00 | 0.58 | 14.76 | 60.28 | -41.44 | 74.92 | 0.6651 | -570.0 | -599.9 | |
| 0.00 | 0.79 | 0.00 | 0.52 | 14.42 | 60.19 | -41.52 | 75.44 | 0.6657 | -679.0 | -546.3 | |
| 0.00 | 0.88 | 0.00 | 0.58 | 13.66 | 60.28 | -41.44 | 76.56 | 0.6635 | -662.0 | -565.5 | |
| 0.00 | 2.02 | 0.00 | 1.34 | 13.57 | 59.84 | -41.88 | 76.77 | 0.6689 | -447.0 | -364.9 | |
| 0.00 | 2.63 | 0.00 | 1.78 | 12.90 | 58.52 | -43.20 | 77.93 | 0.6847 | 744.0 | 608.3 | |
| 0.00 | 0.70 | 0.00 | 0.49 | 13.50 | 56.48 | -45.23 | 77.28 | 0.7101 | 575.0 | 463.5 | |
| 0.00 | 0.53 | 0.00 | 0.37 | 13.08 | 56.06 | -45.66 | 77.93 | 0.7148 | 541.0 | 532.3 | |
| 0.00 | 0.70 | 0.00 | 0.50 | 13.33 | 55.77 | -45.94 | 77.60 | 0.7183 | 542.0 | 377.4 | |
| 0.00 | 0.97 | 0.00 | 0.72 | 10.51 | 52.78 | -48.94 | 81.61 | 0.7517 | 653.0 | 548.5 | |
| 0.00 | 0.97 | 0.00 | 0.73 | 12.36 | 52.06 | -49.65 | 79.18 | 0.7603 | 638.0 | 515.4 | |
| 0.00 | 2.37 | 0.00 | 1.83 | 13.00 | 51.36 | -50.35 | 78.37 | 0.7683 | 508.0 | 418.7 | |
| 0.00 | 1.23 | 0.00 | 0.99 | 14.07 | 49.20 | -52.52 | 77.13 | 0.7918 | 558.0 | 444.9 | |
| 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. | |