| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.16 | 59.57 | 15.80 | 51.28 | 15.68 | 350.17 | -54.13 | 72.58 | 0.8191 | 219.3 | 186.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 1.06 | 19.55 | 358.97 | -45.33 | 65.64 | 0.7380 | -690.0 | -542.1 | |
| 0.00 | 1.27 | 0.00 | 0.93 | 19.22 | 358.58 | -45.72 | 66.20 | 0.7412 | -449.0 | -296.6 | |
| 0.00 | 0.64 | 0.00 | 0.47 | 18.87 | 358.61 | -45.69 | 66.65 | 0.7398 | -599.0 | -481.0 | |
| 0.00 | 1.45 | 0.00 | 1.07 | 18.44 | 358.25 | -46.05 | 67.32 | 0.7425 | -616.0 | -488.3 | |
| 0.00 | 1.09 | 0.00 | 0.91 | 20.10 | 352.33 | -51.97 | 66.84 | 0.8067 | -418.0 | -353.9 | |
| 1.36 | 2.45 | 1.11 | 2.00 | 15.81 | 352.55 | -51.75 | 72.07 | 0.7964 | -652.7 | -625.8 | |
| 0.00 | 1.45 | 0.00 | 1.20 | 16.01 | 352.06 | -52.24 | 71.91 | 0.8016 | -432.0 | -324.1 | |
| 2.27 | 6.72 | 1.89 | 5.58 | 16.51 | 351.82 | -52.48 | 71.35 | 0.8048 | -588.6 | -467.5 | |
| 0.00 | 1.18 | 0.00 | 1.00 | 18.04 | 351.19 | -53.12 | 69.60 | 0.8136 | -328.0 | -313.6 | |
| 0.00 | 0.45 | 0.00 | 0.38 | 16.49 | 351.40 | -52.90 | 71.44 | 0.8089 | -116.0 | -82.6 | |
| 1.27 | 2.18 | 1.10 | 1.89 | 16.16 | 349.92 | -54.38 | 72.12 | 0.8226 | 615.1 | 720.2 | |
| 0.00 | 0.91 | 0.00 | 0.79 | 15.80 | 349.68 | -54.62 | 72.58 | 0.8244 | 703.0 | 617.3 | |
| 0.00 | 0.82 | 0.00 | 0.72 | 15.76 | 349.36 | -54.94 | 72.69 | 0.8273 | 588.0 | 513.6 | |
| 1.91 | 3.18 | 1.68 | 2.80 | 15.21 | 349.14 | -55.16 | 73.37 | 0.8287 | 541.0 | 523.9 | |
| 11.35 | 31.78 | 10.02 | 28.00 | 14.64 | 348.97 | -55.33 | 74.08 | 0.8296 | 765.9 | 476.0 | |
| 0.00 | 0.82 | 0.00 | 0.80 | 17.99 | 345.62 | -58.68 | 70.63 | 0.8632 | 387.0 | 328.4 | |
| 0.00 | 1.73 | 0.00 | 1.68 | 17.74 | 345.63 | -58.67 | 70.92 | 0.8628 | 645.0 | 427.4 | |
| 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. | |