| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.79 | 25.29 | 2.65 | 17.61 | -20.99 | 157.40 | -36.01 | 128.61 | 0.7036 | 290.1 | 160.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.95 | -17.52 | 164.80 | -28.60 | 130.44 | 0.6021 | 724.0 | 618.6 | |
| 0.00 | 1.90 | 0.00 | 1.30 | -22.72 | 160.13 | -33.28 | 132.68 | 0.6908 | 696.0 | 583.4 | |
| 0.00 | 1.72 | 0.00 | 1.16 | -20.50 | 159.57 | -33.83 | 129.61 | 0.6793 | 641.0 | 453.0 | |
| 0.00 | 0.99 | 0.00 | 0.67 | -20.28 | 159.24 | -34.17 | 129.09 | 0.6810 | 664.0 | 537.1 | |
| 0.00 | 0.99 | 0.00 | 0.70 | -22.92 | 158.02 | -35.38 | 131.26 | 0.7117 | 572.0 | 504.1 | |
| 0.00 | 1.08 | 0.00 | 0.73 | -19.44 | 158.74 | -34.66 | 127.67 | 0.6799 | 650.0 | 538.2 | |
| 0.00 | 0.27 | 0.00 | 0.18 | -19.51 | 158.69 | -34.72 | 127.72 | 0.6810 | 728.0 | 638.0 | |
| 2.80 | 4.52 | 1.93 | 3.11 | -21.03 | 158.09 | -35.32 | 129.10 | 0.6976 | 783.6 | 582.3 | |
| 0.00 | 0.72 | 0.00 | 0.51 | -21.27 | 157.09 | -36.31 | 128.64 | 0.7089 | 355.0 | 293.6 | |
| 0.00 | 2.26 | 0.00 | 1.57 | -20.76 | 157.08 | -36.33 | 128.03 | 0.7056 | 572.0 | 452.9 | |
| 0.00 | 0.99 | 0.00 | 0.70 | -20.65 | 156.66 | -36.74 | 127.60 | 0.7089 | 298.0 | 289.7 | |
| 0.00 | 0.36 | 0.00 | 0.25 | -20.71 | 156.24 | -37.17 | 127.37 | 0.7134 | 439.0 | 450.0 | |
| 0.00 | 0.54 | 0.00 | 0.40 | -22.40 | 155.01 | -38.40 | 128.49 | 0.7360 | -548.0 | -467.2 | |
| 0.00 | 1.36 | 0.00 | 0.99 | -22.28 | 154.75 | -38.65 | 128.18 | 0.7376 | -333.0 | -382.4 | |
| 0.00 | 1.72 | 0.00 | 1.24 | -21.03 | 154.57 | -38.84 | 126.61 | 0.7315 | -700.0 | -445.3 | |
| 0.00 | 0.63 | 0.00 | 0.46 | -21.46 | 154.35 | -39.06 | 126.96 | 0.7362 | -686.0 | -454.3 | |
| 0.99 | 3.70 | 0.72 | 2.69 | -21.15 | 154.36 | -39.04 | 126.61 | 0.7342 | -644.5 | -621.6 | |
| 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. | |