| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.74 | 32.24 | 9.99 | 27.60 | -13.52 | 61.90 | 53.61 | 253.88 | 0.8161 | -101.0 | -10.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.78 | -12.29 | 66.50 | 58.21 | 256.08 | 0.8577 | 462.0 | 435.4 | |
| 0.00 | 0.81 | 0.00 | 0.78 | -12.45 | 66.38 | 58.09 | 255.88 | 0.8568 | 408.0 | 419.4 | |
| 3.34 | 5.15 | 3.13 | 4.82 | -12.70 | 65.65 | 57.36 | 255.48 | 0.8506 | 578.3 | 438.9 | |
| 0.00 | 1.54 | 0.00 | 1.39 | -12.65 | 64.31 | 56.03 | 255.34 | 0.8385 | 550.0 | 456.1 | |
| 0.00 | 0.81 | 0.00 | 0.73 | -12.81 | 63.98 | 55.69 | 255.10 | 0.8355 | 526.0 | 482.6 | |
| 0.00 | 1.81 | 0.00 | 1.66 | -18.65 | 63.85 | 55.56 | 248.20 | 0.8437 | 463.0 | 351.4 | |
| 0.00 | 1.26 | 0.00 | 1.15 | -18.69 | 63.42 | 55.13 | 248.06 | 0.8399 | 559.0 | 482.0 | |
| 0.00 | 1.72 | 0.00 | 1.42 | -13.38 | 60.37 | 52.08 | 253.79 | 0.8015 | 195.0 | 236.6 | |
| 8.40 | 11.56 | 6.86 | 9.44 | -13.13 | 59.99 | 51.70 | 254.02 | 0.7973 | -642.3 | -323.6 | |
| 0.00 | 0.36 | 0.00 | 0.29 | -12.26 | 59.60 | 51.31 | 255.02 | 0.7917 | -362.0 | -492.0 | |
| 0.00 | 1.99 | 0.00 | 1.60 | -12.60 | 59.44 | 51.15 | 254.56 | 0.7907 | -648.0 | -633.0 | |
| 0.00 | 2.35 | 0.00 | 1.87 | -12.73 | 58.98 | 50.69 | 254.31 | 0.7861 | -678.0 | -637.2 | |
| 0.00 | 0.99 | 0.00 | 0.81 | -14.57 | 59.48 | 51.19 | 252.12 | 0.7947 | -493.0 | -435.5 | |
| 0.00 | 1.08 | 0.00 | 0.86 | -12.92 | 58.64 | 50.35 | 254.00 | 0.7829 | -606.0 | -587.6 | |
| 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. | |