| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.99 | 51.27 | 6.64 | 28.48 | 19.85 | 63.89 | 4.30 | 351.04 | 0.4545 | 375.7 | 287.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.11 | 0.00 | 0.61 | 17.80 | 69.02 | 9.43 | 339.32 | 0.4435 | -668.0 | -470.8 | |
| 0.00 | 1.54 | 0.00 | 0.88 | 22.17 | 66.61 | 7.02 | 346.79 | 0.4970 | -792.0 | -595.3 | |
| 1.20 | 11.04 | 0.67 | 6.16 | 20.24 | 65.44 | 5.85 | 348.07 | 0.4643 | -702.7 | -659.9 | |
| 1.28 | -3.00 | 0.72 | -3.00 | 20.07 | 65.40 | 5.81 | 348.07 | 0.4617 | -817.9 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 20.63 | 64.15 | 4.56 | 350.79 | 0.4665 | -604.0 | -514.5 | |
| 1.46 | 24.83 | 0.80 | 13.73 | 19.13 | 63.98 | 4.39 | 350.57 | 0.4432 | 929.2 | 692.4 | |
| 2.83 | -6.00 | 1.56 | -6.00 | 19.20 | 63.76 | 4.17 | 351.05 | 0.4436 | 980.0 | 999999 | |
| 1.88 | -6.00 | 1.04 | -6.00 | 19.43 | 63.55 | 3.96 | 351.59 | 0.4467 | 853.0 | 999999 | |
| 3.34 | -6.00 | 1.85 | -6.00 | 19.79 | 63.12 | 3.53 | 352.60 | 0.4513 | 765.4 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.09 | 19.78 | 62.74 | 3.15 | 353.39 | 0.4506 | 1002.0 | 886.5 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 20.45 | 62.75 | 3.16 | 353.54 | 0.4609 | 666.0 | 555.9 | |
| 0.00 | 3.85 | 0.00 | 2.14 | 20.28 | 62.62 | 3.03 | 353.76 | 0.4581 | 901.0 | 767.8 | |
| 0.00 | 2.91 | 0.00 | 1.62 | 20.01 | 62.49 | 2.90 | 353.96 | 0.4537 | 849.0 | 828.2 | |
| 0.00 | 0.77 | 0.00 | 0.43 | 20.61 | 61.24 | 1.65 | 356.65 | 0.4613 | 505.0 | 551.7 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 20.94 | 60.07 | 0.48 | 359.04 | 0.4658 | 501.0 | 464.8 | |
| 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. | |