| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.31 | 78.53 | 15.18 | 73.95 | -20.36 | 259.18 | -52.27 | 119.35 | 0.8526 | 311.8 | 101.9 | |
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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 | 1.11 | -22.24 | 259.64 | -51.82 | 121.56 | 0.8559 | 410.0 | 365.8 | |
| 4.12 | 18.73 | 3.80 | 17.14 | -20.46 | 260.15 | -51.30 | 119.87 | 0.8453 | 566.8 | 657.9 | |
| 12.19 | 29.21 | 11.38 | 27.35 | -20.94 | 259.82 | -51.63 | 120.24 | 0.8496 | 606.4 | 217.9 | |
| 0.00 | 0.63 | 0.00 | 0.57 | -19.96 | 260.18 | -51.27 | 119.33 | 0.8432 | 490.0 | 520.9 | |
| 0.00 | 0.99 | 0.00 | 0.96 | -22.04 | 258.67 | -52.78 | 120.92 | 0.8625 | 323.0 | 236.7 | |
| 0.00 | 0.99 | 0.00 | 0.96 | -21.92 | 258.52 | -52.94 | 120.73 | 0.8632 | 317.0 | 288.4 | |
| 0.00 | 0.99 | 0.00 | 0.96 | -20.99 | 258.30 | -53.16 | 119.65 | 0.8617 | 342.0 | 253.2 | |
| 0.00 | 2.42 | 0.00 | 2.30 | -19.95 | 258.66 | -52.80 | 118.67 | 0.8554 | 473.0 | 318.5 | |
| 0.00 | 18.28 | 0.00 | 17.57 | -19.51 | 258.06 | -53.39 | 117.95 | 0.8586 | -622.0 | -369.5 | |
| 0.00 | 0.90 | 0.00 | 0.87 | -19.54 | 257.44 | -54.01 | 117.73 | 0.8635 | -579.0 | -504.6 | |
| 0.00 | 0.90 | 0.00 | 0.90 | -19.62 | 256.40 | -55.05 | 117.41 | 0.8717 | -492.0 | -441.9 | |
| 0.00 | 0.81 | 0.00 | 0.78 | -18.18 | 257.10 | -54.35 | 116.13 | 0.8619 | -499.0 | -411.9 | |
| 0.00 | 0.90 | 0.00 | 0.87 | -18.04 | 256.95 | -54.50 | 115.91 | 0.8627 | -358.0 | -339.0 | |
| 0.00 | 1.61 | 0.00 | 1.61 | -18.93 | 256.35 | -55.10 | 116.65 | 0.8700 | -386.0 | -315.7 | |
| 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. | |