| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.77 | 0.00 | 9.54 | 13.04 | 259.48 | -6.67 | 210.08 | 0.2090 | 367.6 | 309.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.99 | 0.00 | 1.01 | 18.20 | 270.05 | 3.90 | 343.28 | 0.2255 | -840.0 | -454.4 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 16.10 | 267.47 | 1.32 | 352.97 | 0.1811 | -836.0 | -655.6 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 15.76 | 267.12 | 0.97 | 354.64 | 0.1747 | -942.0 | -809.2 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 16.66 | 266.17 | 0.02 | 359.90 | 0.1894 | -842.0 | -657.1 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 5.49 | 262.49 | -3.67 | 94.65 | 0.0641 | 873.0 | 611.8 | |
| 0.00 | 0.82 | 0.00 | 0.41 | 7.47 | 259.45 | -6.70 | 75.49 | 0.1200 | 854.0 | 661.3 | |
| 0.00 | 2.26 | 0.00 | 1.15 | 16.19 | 258.45 | -7.70 | 35.38 | 0.2233 | 1039.0 | 808.1 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 9.65 | 258.45 | -7.70 | 62.69 | 0.1493 | 949.0 | 691.8 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 14.41 | 257.08 | -9.07 | 45.30 | 0.2157 | 504.0 | 419.1 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 16.66 | 256.76 | -9.39 | 39.47 | 0.2470 | 770.0 | 622.8 | |
| 0.00 | 1.27 | 0.00 | 0.64 | 4.35 | 255.88 | -10.27 | 97.57 | 0.1802 | 912.0 | 755.7 | |
| 0.00 | 1.81 | 0.00 | 0.91 | 4.68 | 255.66 | -10.49 | 95.59 | 0.1832 | 1005.0 | 786.2 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 13.09 | 254.91 | -11.24 | 55.85 | 0.2305 | 805.0 | 656.8 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 21.16 | 247.92 | -18.23 | 47.24 | 0.3990 | 538.0 | 555.0 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 14.28 | 247.14 | -19.01 | 64.16 | 0.3523 | 725.0 | 512.8 | |
| 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. | |