| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.92 | 0.00 | 11.67 | 5.53 | 265.35 | -25.61 | 84.25 | 0.4346 | 236.3 | 217.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 0.83 | 1.67 | 279.48 | -11.48 | 96.88 | 0.2013 | -831.0 | -609.2 | |
| 0.00 | 1.64 | 0.00 | 0.83 | 3.40 | 278.44 | -12.52 | 88.32 | 0.2175 | -787.0 | -643.0 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 0.80 | 278.27 | -12.69 | 100.03 | 0.2241 | -845.0 | -655.3 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 5.14 | 276.39 | -14.56 | 81.54 | 0.2543 | -716.0 | -574.4 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 1.57 | 273.91 | -17.05 | 94.76 | 0.2954 | -831.0 | -713.0 | |
| 0.00 | 2.27 | 0.00 | 1.23 | 11.04 | 267.93 | -23.03 | 69.67 | 0.4111 | 773.0 | 605.4 | |
| 0.00 | 0.64 | 0.00 | 0.35 | 10.59 | 267.36 | -23.60 | 71.09 | 0.4177 | 718.0 | 618.3 | |
| 0.00 | 1.64 | 0.00 | 0.90 | 11.53 | 266.43 | -24.53 | 69.60 | 0.4358 | 154.0 | 280.2 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 9.65 | 265.05 | -25.91 | 74.51 | 0.4489 | 793.0 | 622.2 | |
| 0.00 | 0.73 | 0.00 | 0.40 | 1.89 | 263.74 | -27.21 | 91.90 | 0.4592 | 586.0 | 499.8 | |
| 0.00 | 1.82 | 0.00 | 1.04 | 8.67 | 261.18 | -29.78 | 78.03 | 0.5039 | 797.0 | 627.7 | |
| 0.00 | 1.09 | 0.00 | 0.63 | 9.21 | 260.66 | -30.29 | 77.14 | 0.5128 | 859.0 | 663.6 | |
| 0.00 | 1.91 | 0.00 | 1.13 | -1.18 | 258.39 | -32.56 | 97.01 | 0.5443 | 598.0 | 533.9 | |
| 0.00 | 0.27 | 0.00 | 0.16 | 7.21 | 258.12 | -32.84 | 81.52 | 0.5460 | 689.0 | 666.7 | |
| 0.00 | 0.36 | 0.00 | 0.22 | 7.75 | 257.60 | -33.36 | 80.64 | 0.5543 | 411.0 | 296.5 | |
| 0.00 | 0.91 | 0.00 | 0.56 | -2.10 | 255.20 | -35.76 | 97.85 | 0.5917 | 612.0 | 453.3 | |
| 0.00 | 1.00 | 0.00 | 0.64 | 8.32 | 251.40 | -39.56 | 80.70 | 0.6409 | 580.0 | 472.6 | |
| 0.00 | 1.00 | 0.00 | 0.67 | 4.41 | 248.92 | -42.04 | 86.85 | 0.6709 | 693.0 | 624.5 | |
| 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. | |