| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.14 | 23.50 | 0.65 | 13.19 | -8.52 | 9.80 | 28.11 | 263.22 | 0.4709 | 331.6 | 306.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.71 | -8.59 | 12.14 | 30.45 | 263.38 | 0.5064 | 597.0 | 477.3 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -8.26 | 12.11 | 30.42 | 264.04 | 0.5058 | 570.0 | 507.0 | |
| 0.00 | 0.88 | 0.00 | 0.50 | -7.82 | 11.79 | 30.10 | 264.88 | 0.5009 | 595.0 | 492.2 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -8.85 | 11.77 | 30.08 | 262.83 | 0.5012 | 730.0 | 700.1 | |
| 1.14 | 5.37 | 0.65 | 3.06 | -8.23 | 11.54 | 29.85 | 264.06 | 0.4973 | 1024.1 | 719.0 | |
| 0.00 | 2.47 | 0.00 | 1.41 | -8.47 | 11.53 | 29.84 | 263.57 | 0.4973 | 805.0 | 659.5 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -8.57 | 11.40 | 29.71 | 263.36 | 0.4954 | 841.0 | 709.8 | |
| 0.00 | 1.41 | 0.00 | 0.80 | -8.95 | 11.05 | 29.36 | 262.55 | 0.4904 | 759.0 | 594.1 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -8.74 | 10.99 | 29.30 | 262.97 | 0.4894 | 845.0 | 688.6 | |
| 0.00 | 1.14 | 0.00 | 0.64 | -9.92 | 8.99 | 27.30 | 260.14 | 0.4604 | 654.0 | 444.2 | |
| 0.00 | 1.59 | 0.00 | 0.86 | -7.50 | 6.57 | 24.88 | 265.28 | 0.4204 | -756.0 | -525.7 | |
| 0.00 | 2.11 | 0.00 | 1.15 | -7.64 | 6.18 | 24.49 | 264.92 | 0.4143 | -807.0 | -780.0 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -8.14 | 5.65 | 23.96 | 263.63 | 0.4062 | -649.0 | -478.6 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -8.24 | 5.45 | 23.76 | 263.36 | 0.4032 | -751.0 | -636.1 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -11.85 | 4.83 | 23.14 | 254.21 | 0.4014 | 759.0 | 521.8 | |
| 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. | |