| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.87 | 17.66 | 0.64 | 12.54 | -9.43 | 21.06 | 46.06 | 263.75 | 0.7155 | 34.3 | 139.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 0.83 | -8.59 | 23.48 | 48.47 | 264.91 | 0.7455 | 428.0 | 339.4 | |
| 0.00 | 0.69 | 0.00 | 0.51 | -9.28 | 23.56 | 48.55 | 263.99 | 0.7461 | 505.0 | 452.8 | |
| 0.00 | 3.38 | 0.00 | 2.50 | -9.05 | 23.47 | 48.46 | 264.31 | 0.7452 | 706.0 | 624.1 | |
| 0.87 | 2.00 | 0.64 | 1.47 | -9.54 | 23.33 | 48.32 | 263.65 | 0.7435 | 519.8 | 501.5 | |
| 0.00 | 1.21 | 0.00 | 0.88 | -9.44 | 22.41 | 47.40 | 263.80 | 0.7328 | 513.0 | 497.4 | |
| 0.00 | 1.30 | 0.00 | 0.93 | -8.07 | 21.61 | 46.60 | 265.72 | 0.7237 | -437.0 | -364.1 | |
| 0.00 | 1.30 | 0.00 | 0.93 | -9.71 | 21.48 | 46.47 | 263.46 | 0.7217 | -428.0 | -309.6 | |
| 0.00 | 0.69 | 0.00 | 0.49 | -9.54 | 21.27 | 46.27 | 263.68 | 0.7193 | -423.0 | -401.0 | |
| 0.00 | 0.95 | 0.00 | 0.68 | -9.56 | 21.06 | 46.05 | 263.66 | 0.7167 | -463.0 | -458.6 | |
| 0.00 | 1.21 | 0.00 | 0.86 | -9.21 | 20.95 | 45.95 | 264.16 | 0.7155 | -346.0 | -365.5 | |
| 0.00 | 0.69 | 0.00 | 0.48 | -9.72 | 19.24 | 44.23 | 263.46 | 0.6944 | 623.0 | 563.9 | |
| 0.00 | 1.47 | 0.00 | 1.00 | -9.91 | 18.80 | 43.80 | 263.19 | 0.6890 | 627.0 | 419.4 | |
| 0.00 | 0.69 | 0.00 | 0.42 | -11.36 | 11.06 | 36.05 | 260.57 | 0.5871 | -514.0 | -460.1 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -11.52 | 7.90 | 32.89 | 259.91 | 0.5426 | -656.0 | -560.3 | |
| 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. | |