| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.49 | 22.60 | 0.90 | 13.70 | 17.95 | 90.55 | -25.28 | 45.01 | 0.5768 | -477.4 | -489.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.49 | 0.00 | 0.90 | 19.96 | 92.96 | -22.87 | 39.72 | 0.5738 | 665.0 | 582.9 | |
| 0.00 | 2.45 | 0.00 | 1.48 | 18.21 | 91.50 | -24.34 | 43.61 | 0.5697 | -736.0 | -600.0 | |
| 0.00 | 0.53 | 0.00 | 0.32 | 17.99 | 91.39 | -24.44 | 44.02 | 0.5685 | -733.0 | -629.7 | |
| 0.00 | 2.36 | 0.00 | 1.42 | 17.90 | 91.27 | -24.57 | 44.28 | 0.5689 | -759.0 | -757.0 | |
| 0.00 | 1.23 | 0.00 | 0.74 | 17.85 | 91.00 | -24.84 | 44.65 | 0.5711 | -710.0 | -597.9 | |
| 0.00 | 1.93 | 0.00 | 1.17 | 18.06 | 90.76 | -25.08 | 44.66 | 0.5755 | -740.0 | -657.4 | |
| 0.00 | 1.05 | 0.00 | 0.64 | 18.10 | 90.54 | -25.29 | 44.84 | 0.5781 | -526.0 | -444.3 | |
| 0.00 | 0.88 | 0.00 | 0.52 | 16.56 | 90.63 | -25.21 | 46.77 | 0.5624 | -698.0 | -603.9 | |
| 0.00 | 2.19 | 0.00 | 1.33 | 17.88 | 90.37 | -25.47 | 45.32 | 0.5777 | -697.0 | -609.4 | |
| 0.00 | 1.31 | 0.00 | 0.80 | 17.99 | 90.14 | -25.69 | 45.43 | 0.5811 | -643.0 | -536.3 | |
| 1.49 | 4.55 | 0.90 | 2.76 | 17.64 | 90.02 | -25.81 | 46.02 | 0.5790 | -793.5 | -722.0 | |
| 0.00 | 0.79 | 0.00 | 0.48 | 17.87 | 89.88 | -25.96 | 45.86 | 0.5826 | -393.0 | -366.2 | |
| 0.00 | 0.96 | 0.00 | 0.60 | 18.19 | 88.42 | -27.42 | 47.00 | 0.6004 | -589.0 | -511.5 | |
| 0.00 | 0.88 | 0.00 | 0.54 | 16.56 | 87.16 | -28.68 | 50.38 | 0.5994 | 638.0 | 461.5 | |
| 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. | |