| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.21 | 0.00 | 11.34 | -10.23 | 335.46 | -30.15 | 114.71 | 0.5463 | -677.5 | -571.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.21 | 0.00 | 0.70 | -9.93 | 336.99 | -28.62 | 115.29 | 0.5239 | -817.0 | -655.2 | |
| 0.00 | 2.67 | 0.00 | 1.58 | -12.07 | 336.13 | -29.48 | 118.26 | 0.5485 | -734.0 | -580.3 | |
| 0.00 | 4.13 | 0.00 | 2.42 | -10.01 | 336.33 | -29.28 | 114.93 | 0.5333 | -729.0 | -633.0 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -10.42 | 336.08 | -29.53 | 115.44 | 0.5390 | -742.0 | -642.3 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -9.94 | 335.50 | -30.11 | 114.23 | 0.5440 | -766.0 | -508.9 | |
| 0.00 | 1.98 | 0.00 | 1.18 | -10.84 | 335.26 | -30.35 | 115.57 | 0.5523 | -708.0 | -614.9 | |
| 0.00 | 0.34 | 0.00 | 0.20 | -10.19 | 335.33 | -30.28 | 114.54 | 0.5476 | -513.0 | -388.8 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -9.56 | 335.26 | -30.35 | 113.40 | 0.5451 | -842.0 | -658.9 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -10.32 | 335.14 | -30.47 | 114.62 | 0.5508 | -645.0 | -499.3 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -9.39 | 334.75 | -30.86 | 112.78 | 0.5510 | -710.0 | -587.3 | |
| 0.00 | 0.78 | 0.00 | 0.46 | -10.63 | 334.09 | -31.52 | 114.41 | 0.5665 | -661.0 | -495.2 | |
| 0.00 | 0.86 | 0.00 | 0.51 | -7.65 | 334.00 | -31.61 | 109.35 | 0.5528 | -628.0 | -526.8 | |
| 0.00 | 1.12 | 0.00 | 0.67 | -9.42 | 333.58 | -32.03 | 112.11 | 0.5669 | -458.0 | -386.5 | |
| 0.00 | 0.86 | 0.00 | 0.52 | -9.82 | 333.54 | -32.07 | 112.74 | 0.5695 | -532.0 | -419.0 | |
| 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. | |