| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.76 | 32.51 | 5.93 | 22.93 | -14.90 | 248.62 | -40.03 | 119.19 | 0.7133 | 47.2 | -169.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.40 | 11.86 | 3.65 | 8.03 | -15.33 | 251.64 | -37.01 | 121.57 | 0.6837 | 920.7 | 560.3 | |
| 3.36 | -1.00 | 2.28 | -1.00 | -15.52 | 251.60 | -37.06 | 121.79 | 0.6854 | 720.8 | 999999 | |
| 0.00 | 2.92 | 0.00 | 1.95 | -13.90 | 251.81 | -36.85 | 119.81 | 0.6732 | 706.0 | 589.6 | |
| 0.00 | 0.89 | 0.00 | 0.59 | -13.78 | 251.63 | -37.02 | 119.55 | 0.6745 | 587.0 | 506.0 | |
| 0.00 | 1.51 | 0.00 | 1.08 | -13.91 | 247.23 | -41.42 | 117.04 | 0.7233 | -633.0 | -618.8 | |
| 0.00 | 1.51 | 0.00 | 1.08 | -13.96 | 247.01 | -41.64 | 116.98 | 0.7259 | -682.0 | -534.7 | |
| 0.00 | 0.62 | 0.00 | 0.45 | -15.48 | 246.53 | -42.13 | 118.60 | 0.7386 | -503.0 | -507.3 | |
| 0.00 | 1.33 | 0.00 | 0.96 | -14.46 | 246.73 | -41.92 | 117.46 | 0.7314 | -188.0 | -135.9 | |
| 0.00 | 1.15 | 0.00 | 0.83 | -13.98 | 246.72 | -41.94 | 116.85 | 0.7292 | -306.0 | -419.2 | |
| 0.00 | 1.95 | 0.00 | 1.43 | -15.50 | 246.27 | -42.39 | 118.49 | 0.7414 | -676.0 | -571.0 | |
| 0.00 | 1.15 | 0.00 | 0.84 | -14.45 | 246.48 | -42.17 | 117.31 | 0.7340 | -495.0 | -499.0 | |
| 0.00 | 1.86 | 0.00 | 1.38 | -15.61 | 245.72 | -42.93 | 118.32 | 0.7475 | -562.0 | -408.7 | |
| 0.00 | 1.24 | 0.00 | 0.92 | -14.85 | 245.58 | -43.07 | 117.31 | 0.7453 | -779.0 | -693.1 | |
| 0.00 | 1.95 | 0.00 | 1.45 | -15.02 | 245.45 | -43.20 | 117.46 | 0.7474 | -611.0 | -567.0 | |
| 0.00 | 1.42 | 0.00 | 1.06 | -15.04 | 244.88 | -43.77 | 117.18 | 0.7533 | -616.0 | -529.8 | |
| 0.00 | 0.71 | 0.00 | 0.54 | -14.96 | 244.34 | -44.31 | 116.80 | 0.7584 | 313.0 | 279.1 | |
| 0.00 | 0.44 | 0.00 | 0.34 | -14.65 | 243.50 | -45.15 | 116.00 | 0.7655 | 429.0 | 366.4 | |
| 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. | |