| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.35 | 51.81 | 14.29 | 64.48 | 16.13 | 23.00 | -67.40 | 75.23 | 0.9183 | 45.4 | 45.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 1.31 | 16.69 | 26.00 | -64.41 | 74.61 | 0.8978 | -584.0 | -511.1 | |
| 0.99 | 2.79 | 1.11 | 3.12 | 16.40 | 25.96 | -64.45 | 74.94 | 0.8981 | -503.9 | -449.2 | |
| 0.54 | 1.89 | 0.61 | 2.14 | 16.83 | 25.53 | -64.87 | 74.46 | 0.9012 | -480.8 | -443.6 | |
| 0.00 | 5.23 | 0.00 | 5.99 | 16.61 | 25.22 | -65.18 | 74.71 | 0.9035 | -385.0 | -295.4 | |
| 1.71 | 3.06 | 1.96 | 3.51 | 16.17 | 25.20 | -65.21 | 75.20 | 0.9036 | -192.3 | -189.9 | |
| 0.00 | 3.88 | 0.00 | 4.57 | 16.97 | 24.44 | -65.97 | 74.32 | 0.9090 | -330.0 | -145.4 | |
| 0.00 | 1.44 | 0.00 | 1.73 | 16.64 | 23.95 | -66.45 | 74.69 | 0.9124 | 267.0 | 214.5 | |
| 0.00 | 1.80 | 0.00 | 2.11 | 15.47 | 24.56 | -65.85 | 75.97 | 0.9082 | -204.0 | -115.3 | |
| 2.07 | 4.51 | 2.54 | 5.53 | 16.58 | 23.42 | -66.98 | 74.75 | 0.9160 | -184.5 | -38.4 | |
| 0.00 | 1.35 | 0.00 | 1.65 | 16.31 | 23.53 | -66.87 | 75.05 | 0.9153 | 146.0 | 140.7 | |
| 0.00 | 0.81 | 0.00 | 1.02 | 16.52 | 22.80 | -67.60 | 74.82 | 0.9201 | 317.0 | 333.9 | |
| 0.00 | 2.16 | 0.00 | 2.66 | 15.34 | 23.28 | -67.12 | 76.11 | 0.9170 | 283.0 | 236.6 | |
| 3.61 | 11.27 | 4.63 | 14.44 | 15.42 | 22.22 | -68.18 | 76.01 | 0.9239 | 433.0 | 309.6 | |
| 0.00 | 3.70 | 0.00 | 5.16 | 16.31 | 20.20 | -70.20 | 75.02 | 0.9363 | 430.0 | 377.5 | |
| 0.99 | 2.43 | 1.38 | 3.39 | 15.85 | 20.29 | -70.11 | 75.52 | 0.9358 | 429.7 | 409.1 | |
| 1.44 | 2.97 | 2.06 | 4.24 | 16.22 | 19.70 | -70.71 | 75.10 | 0.9393 | 118.9 | 106.8 | |
| 0.00 | 1.35 | 0.00 | 1.91 | 15.71 | 19.93 | -70.48 | 75.65 | 0.9380 | 19.0 | 6.9 | |
| 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. | |