| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.96 | 375.22 | 36.64 | 249.89 | -21.15 | 16.78 | 32.70 | 228.97 | 0.6702 | 890.5 | 324.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.40 | 0.00 | 0.93 | -17.16 | 19.37 | 35.29 | 236.01 | 0.6681 | 765.0 | 690.4 | |
| 27.96 | 358.09 | 18.72 | 238.83 | -21.23 | 17.22 | 33.15 | 229.26 | 0.6750 | 1087.9 | 340.5 | |
| 0.00 | 0.87 | 0.00 | 0.56 | -18.18 | 16.41 | 32.33 | 232.39 | 0.6437 | -472.0 | -387.2 | |
| 0.26 | -2.00 | 0.17 | -2.00 | -20.53 | 16.78 | 32.71 | 229.74 | 0.6654 | 1280.3 | 999999 | |
| 25.87 | -2.00 | 17.17 | -2.00 | -21.06 | 16.65 | 32.57 | 228.98 | 0.6681 | 1345.0 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.56 | -18.48 | 16.02 | 31.95 | 231.67 | 0.6420 | 59.0 | 101.5 | |
| 0.87 | -2.00 | 0.58 | -2.00 | -20.90 | 16.19 | 32.11 | 228.79 | 0.6624 | 1275.5 | 999999 | |
| 0.00 | 0.44 | 0.00 | 0.29 | -21.73 | 15.03 | 30.95 | 226.79 | 0.6579 | 385.0 | 404.0 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -20.75 | 14.69 | 30.61 | 227.67 | 0.6464 | 498.0 | 474.2 | |
| 0.00 | 1.05 | 0.00 | 0.70 | -23.71 | 15.19 | 31.11 | 224.63 | 0.6757 | 512.0 | 488.4 | |
| 0.00 | 2.18 | 0.00 | 1.42 | -21.70 | 14.39 | 30.31 | 226.25 | 0.6514 | 568.0 | 348.7 | |
| 0.00 | 0.79 | 0.00 | 0.51 | -21.90 | 14.40 | 30.32 | 226.02 | 0.6532 | 230.0 | 326.7 | |
| 0.00 | 1.75 | 0.00 | 1.13 | -21.49 | 14.22 | 30.15 | 226.35 | 0.6481 | 158.0 | 141.1 | |
| 0.00 | 1.75 | 0.00 | 1.12 | -21.15 | 13.48 | 29.40 | 226.08 | 0.6380 | -455.0 | -454.5 | |
| 0.00 | 1.92 | 0.00 | 1.23 | -21.41 | 13.32 | 29.24 | 225.61 | 0.6387 | -611.0 | -444.4 | |
| 0.00 | 0.70 | 0.00 | 0.44 | -22.32 | 9.55 | 25.47 | 220.71 | 0.6121 | -469.0 | -483.2 | |
| 0.00 | 0.96 | 0.00 | 0.59 | -24.05 | 6.21 | 22.13 | 215.02 | 0.6017 | -590.0 | -492.4 | |
| 0.00 | 1.31 | 0.00 | 0.84 | -28.51 | 4.12 | 20.04 | 208.34 | 0.6366 | -292.0 | -335.0 | |
| 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. | |