| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.19 | 34.07 | 14.82 | 35.25 | -20.52 | 79.24 | -55.72 | 118.19 | 0.8791 | 21.1 | 7.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.25 | 2.86 | 1.19 | 2.71 | -20.55 | 82.51 | -52.45 | 119.51 | 0.8551 | 606.1 | 499.4 | |
| 0.62 | 1.78 | 0.60 | 1.71 | -20.27 | 82.01 | -52.96 | 118.99 | 0.8580 | 432.1 | 411.8 | |
| 0.98 | 2.32 | 0.95 | 2.24 | -20.49 | 81.84 | -53.12 | 119.16 | 0.8601 | 318.6 | 247.5 | |
| 0.00 | 0.80 | 0.00 | 0.80 | -21.29 | 80.99 | -53.97 | 119.66 | 0.8692 | 520.0 | 449.3 | |
| 0.00 | 0.71 | 0.00 | 0.70 | -20.76 | 81.16 | -53.81 | 119.17 | 0.8662 | 342.0 | 282.4 | |
| 0.00 | 0.71 | 0.00 | 0.66 | -17.90 | 82.46 | -52.50 | 116.59 | 0.8463 | 414.0 | 437.2 | |
| 0.45 | 1.61 | 0.46 | 1.64 | -21.45 | 80.11 | -54.85 | 119.48 | 0.8762 | 538.2 | 442.7 | |
| 3.39 | 5.35 | 3.46 | 5.46 | -21.06 | 79.99 | -54.97 | 119.02 | 0.8758 | 314.4 | 166.5 | |
| 0.00 | 0.62 | 0.00 | 0.61 | -18.90 | 80.83 | -54.13 | 117.03 | 0.8627 | 378.0 | 346.1 | |
| 0.00 | 0.80 | 0.00 | 0.81 | -20.32 | 79.94 | -55.02 | 118.21 | 0.8740 | -392.0 | -423.7 | |
| 0.00 | 0.45 | 0.00 | 0.46 | -20.03 | 78.95 | -56.01 | 117.52 | 0.8803 | -500.0 | -443.4 | |
| 0.00 | 1.16 | 0.00 | 1.21 | -20.17 | 78.87 | -56.09 | 117.65 | 0.8813 | -538.0 | -430.6 | |
| 6.43 | 12.58 | 6.80 | 13.29 | -20.01 | 78.20 | -56.76 | 117.23 | 0.8857 | -465.2 | -371.4 | |
| 1.07 | 2.32 | 1.36 | 2.95 | -22.39 | 73.52 | -61.44 | 118.09 | 0.9222 | 194.1 | 106.4 | |
| 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. | |