| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.17 | 231.81 | 43.10 | 199.40 | -19.63 | 107.29 | -48.57 | 120.26 | 0.8196 | 686.6 | 337.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.80 | 0.00 | 0.69 | -22.90 | 109.15 | -46.70 | 124.79 | 0.8185 | -195.0 | -162.0 | |
| 0.00 | 0.62 | 0.00 | 0.52 | -19.79 | 108.98 | -46.87 | 121.27 | 0.8057 | -291.0 | -171.1 | |
| 1.16 | 7.14 | 1.03 | 6.31 | -22.48 | 107.49 | -48.36 | 123.48 | 0.8301 | 646.3 | 513.1 | |
| 0.00 | 0.27 | 0.00 | 0.24 | -22.70 | 107.34 | -48.52 | 123.64 | 0.8323 | 268.0 | 226.7 | |
| 0.00 | 2.95 | 0.00 | 2.49 | -19.83 | 108.26 | -47.60 | 120.95 | 0.8122 | 792.0 | 585.5 | |
| 0.00 | 0.98 | 0.00 | 0.87 | -22.11 | 107.07 | -48.78 | 122.88 | 0.8319 | 565.0 | 501.5 | |
| 0.00 | 0.36 | 0.00 | 0.30 | -19.63 | 107.85 | -48.00 | 120.53 | 0.8148 | 617.0 | 585.0 | |
| 19.73 | 87.21 | 16.54 | 72.86 | -18.68 | 108.08 | -47.77 | 119.57 | 0.8088 | 929.0 | 488.9 | |
| 8.12 | 118.10 | 7.09 | 103.14 | -20.65 | 107.09 | -48.77 | 121.29 | 0.8256 | 683.1 | 242.2 | |
| 0.00 | 0.80 | 0.00 | 0.71 | -21.14 | 106.57 | -49.28 | 121.58 | 0.8320 | -245.0 | -217.8 | |
| 16.60 | -9.00 | 14.47 | -9.00 | -19.90 | 106.82 | -49.04 | 120.34 | 0.8248 | 892.3 | 999999 | |
| 4.02 | 7.32 | 3.47 | 6.33 | -19.14 | 106.79 | -49.07 | 119.47 | 0.8220 | 701.2 | 454.9 | |
| 0.00 | 1.52 | 0.00 | 1.40 | -19.70 | 104.22 | -51.63 | 118.94 | 0.8456 | 531.0 | 422.8 | |
| 0.00 | 0.62 | 0.00 | 0.57 | -18.01 | 104.24 | -51.61 | 117.08 | 0.8394 | -235.0 | -153.9 | |
| 0.54 | 1.43 | 0.50 | 1.34 | -17.99 | 102.84 | -53.02 | 116.48 | 0.8509 | -524.0 | -523.8 | |
| 0.00 | 0.98 | 0.00 | 0.94 | -18.76 | 102.11 | -53.74 | 117.04 | 0.8593 | -375.0 | -255.4 | |
| 0.00 | 0.71 | 0.00 | 0.69 | -18.13 | 101.47 | -54.38 | 116.11 | 0.8623 | -243.0 | -191.8 | |
| 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. | |