| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.13 | 227.02 | 48.24 | 210.36 | -19.58 | 107.27 | -51.90 | 118.69 | 0.8471 | 617.2 | 269.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.98 | 0.00 | 0.91 | -23.07 | 109.16 | -50.02 | 123.30 | 0.8456 | -263.0 | -275.2 | |
| 0.89 | 6.52 | 0.85 | 6.19 | -22.34 | 107.55 | -51.62 | 121.79 | 0.8551 | 587.9 | 436.9 | |
| 0.00 | 1.79 | 0.00 | 1.62 | -19.75 | 108.14 | -51.04 | 119.24 | 0.8408 | 531.0 | 456.9 | |
| 0.00 | 1.25 | 0.00 | 1.20 | -22.09 | 106.99 | -52.18 | 121.28 | 0.8585 | 393.0 | 328.7 | |
| 0.00 | 1.07 | 0.00 | 0.98 | -19.52 | 107.72 | -51.45 | 118.82 | 0.8434 | 398.0 | 400.4 | |
| 20.62 | 81.51 | 18.61 | 73.27 | -18.67 | 107.99 | -51.18 | 117.99 | 0.8380 | 822.9 | 433.3 | |
| 8.21 | 126.86 | 7.72 | 119.22 | -20.56 | 107.13 | -52.04 | 119.69 | 0.8518 | 644.6 | 182.1 | |
| 0.00 | 0.71 | 0.00 | 0.66 | -19.26 | 107.37 | -51.80 | 118.38 | 0.8453 | 487.0 | 483.8 | |
| 9.02 | -7.00 | 8.48 | -7.00 | -20.14 | 106.91 | -52.26 | 119.14 | 0.8521 | 699.3 | 999999 | |
| 8.30 | -7.00 | 7.79 | -7.00 | -19.78 | 106.87 | -52.30 | 118.73 | 0.8511 | 736.5 | 999999 | |
| 4.55 | -7.00 | 4.24 | -7.00 | -19.11 | 106.92 | -52.25 | 118.02 | 0.8484 | 618.1 | 999999 | |
| 0.00 | 1.07 | 0.00 | 1.01 | -19.31 | 106.30 | -52.87 | 117.98 | 0.8541 | 120.0 | 122.2 | |
| 0.00 | 1.34 | 0.00 | 1.33 | -19.67 | 104.43 | -54.75 | 117.62 | 0.8698 | 506.0 | 433.5 | |
| 0.00 | 0.62 | 0.00 | 0.62 | -18.07 | 104.26 | -54.91 | 115.82 | 0.8662 | -231.0 | -220.4 | |
| 0.00 | 1.34 | 0.00 | 1.34 | -18.27 | 103.61 | -55.56 | 115.80 | 0.8719 | -389.0 | -324.8 | |
| 0.00 | 0.71 | 0.00 | 0.73 | -18.29 | 103.08 | -56.09 | 115.63 | 0.8759 | -350.0 | -294.5 | |
| 0.54 | 1.25 | 0.55 | 1.28 | -17.92 | 102.86 | -56.31 | 115.15 | 0.8765 | -612.0 | -510.9 | |
| 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. | |