| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.62 | 0.00 | 9.67 | -19.89 | 163.25 | -6.24 | 160.65 | 0.2908 | -695.0 | -528.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.66 | 0.00 | 1.34 | -12.88 | 174.59 | 5.10 | 212.48 | 0.1622 | -804.0 | -492.4 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -25.39 | 167.50 | -1.99 | 174.85 | 0.3503 | -769.0 | -576.5 | |
| 0.00 | 1.06 | 0.00 | 0.56 | -24.08 | 166.57 | -2.92 | 171.87 | 0.3305 | -782.0 | -625.3 | |
| 0.00 | 1.51 | 0.00 | 0.75 | -9.46 | 162.94 | -6.54 | 124.43 | 0.1369 | -896.0 | -701.1 | |
| 0.00 | 1.51 | 0.00 | 0.81 | -26.41 | 161.98 | -7.51 | 162.21 | 0.3846 | -804.0 | -628.9 | |
| 0.00 | 1.24 | 0.00 | 0.64 | -19.81 | 161.90 | -7.59 | 154.05 | 0.2851 | -899.0 | -698.4 | |
| 0.00 | 0.80 | 0.00 | 0.41 | -16.96 | 161.71 | -7.78 | 147.97 | 0.2451 | -893.0 | -683.6 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -16.99 | 161.52 | -7.97 | 147.41 | 0.2472 | -780.0 | -601.3 | |
| 0.00 | 1.24 | 0.00 | 0.67 | -27.76 | 160.44 | -9.05 | 160.21 | 0.4127 | 707.0 | 562.6 | |
| 0.00 | 1.69 | 0.00 | 0.87 | -19.51 | 160.43 | -9.06 | 149.36 | 0.2924 | -728.0 | -622.7 | |
| 0.00 | 1.69 | 0.00 | 0.87 | -17.79 | 159.08 | -10.41 | 142.18 | 0.2817 | -763.0 | -541.0 | |
| 0.00 | 1.15 | 0.00 | 0.61 | -23.47 | 158.13 | -11.35 | 150.35 | 0.3666 | -907.0 | -779.3 | |
| 0.00 | 0.53 | 0.00 | 0.28 | -23.66 | 157.95 | -11.54 | 150.24 | 0.3706 | -727.0 | -632.7 | |
| 0.00 | 1.24 | 0.00 | 0.66 | -23.49 | 157.76 | -11.72 | 149.61 | 0.3699 | -685.0 | -524.1 | |
| 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. | |