| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.43 | 87.72 | 7.88 | 48.44 | -10.72 | 139.92 | -19.51 | 131.53 | 0.4411 | 235.6 | 368.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 0.44 | -11.79 | 140.99 | -18.45 | 135.06 | 0.4404 | 782.0 | 688.0 | |
| 1.94 | 60.71 | 1.06 | 33.20 | -9.80 | 140.47 | -18.96 | 130.85 | 0.4251 | 1211.8 | 581.5 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -15.70 | 140.00 | -19.44 | 139.40 | 0.4943 | 594.0 | 462.0 | |
| 2.46 | -2.00 | 1.35 | -2.00 | -9.99 | 140.40 | -19.04 | 131.08 | 0.4280 | 986.7 | 999999 | |
| 6.42 | -2.00 | 3.50 | -2.00 | -9.21 | 140.41 | -19.02 | 129.68 | 0.4199 | 1065.3 | 999999 | |
| 3.08 | -2.00 | 1.68 | -2.00 | -9.58 | 140.39 | -19.05 | 130.33 | 0.4239 | 1178.7 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.61 | -16.55 | 139.68 | -19.76 | 140.09 | 0.5071 | 639.0 | 490.5 | |
| 0.53 | 10.38 | 0.29 | 5.76 | -11.89 | 139.84 | -19.59 | 133.51 | 0.4543 | 948.5 | 705.4 | |
| 0.00 | 1.23 | 0.00 | 0.70 | -15.20 | 138.72 | -20.71 | 136.91 | 0.5017 | -814.0 | -669.9 | |
| 0.00 | 1.23 | 0.00 | 0.71 | -15.42 | 138.07 | -21.37 | 136.33 | 0.5108 | -741.0 | -570.1 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -13.17 | 138.19 | -21.24 | 133.20 | 0.4860 | -877.0 | -666.9 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -14.30 | 137.95 | -21.49 | 134.57 | 0.5003 | -781.0 | -651.5 | |
| 0.00 | 1.58 | 0.00 | 0.90 | -14.01 | 137.91 | -21.52 | 134.10 | 0.4977 | -691.0 | -517.5 | |
| 0.00 | 1.41 | 0.00 | 0.80 | -12.83 | 137.99 | -21.44 | 132.41 | 0.4847 | -825.0 | -752.2 | |
| 0.00 | 3.96 | 0.00 | 2.26 | -14.02 | 137.75 | -21.69 | 133.89 | 0.4996 | -692.0 | -615.7 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -15.34 | 137.57 | -21.87 | 135.58 | 0.5152 | -666.0 | -523.4 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -12.31 | 136.01 | -23.43 | 129.10 | 0.5025 | -558.0 | -416.6 | |
| 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. | |