| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.28 | 292.41 | 80.17 | 342.19 | -8.36 | 249.09 | -63.34 | 101.97 | 0.9055 | 293.2 | -104.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.45 | 284.44 | 2.67 | 332.68 | -8.80 | 250.83 | -61.61 | 102.80 | 0.8933 | 611.9 | -97.4 | |
| 3.71 | -1.00 | 4.09 | -1.00 | -8.60 | 250.55 | -61.88 | 102.53 | 0.8951 | 637.8 | 999999 | |
| 0.00 | 1.45 | 0.00 | 1.57 | -6.97 | 250.72 | -61.71 | 100.76 | 0.8916 | 315.0 | 305.6 | |
| 1.09 | -1.00 | 1.22 | -1.00 | -8.18 | 250.08 | -62.35 | 101.96 | 0.8981 | 635.3 | 999999 | |
| 5.16 | -1.00 | 5.84 | -1.00 | -8.73 | 249.85 | -62.58 | 102.52 | 0.9006 | -13.6 | 999999 | |
| 3.44 | -1.00 | 3.87 | -1.00 | -7.91 | 249.88 | -62.55 | 101.63 | 0.8992 | 763.6 | 999999 | |
| 6.61 | -1.00 | 7.57 | -1.00 | -8.64 | 249.47 | -62.96 | 102.34 | 0.9032 | 193.5 | 999999 | |
| 12.13 | -1.00 | 13.90 | -1.00 | -8.30 | 249.37 | -63.07 | 101.96 | 0.9035 | 470.4 | 999999 | |
| 0.00 | 1.54 | 0.00 | 1.83 | -9.89 | 248.71 | -63.72 | 103.55 | 0.9104 | -507.0 | -523.1 | |
| 15.58 | -1.00 | 17.90 | -1.00 | -7.85 | 249.22 | -63.21 | 101.43 | 0.9040 | 676.0 | 999999 | |
| 1.72 | -1.00 | 2.00 | -1.00 | -7.48 | 248.84 | -63.59 | 100.96 | 0.9063 | 371.8 | 999999 | |
| 0.00 | 1.09 | 0.00 | 1.29 | -8.45 | 248.41 | -64.02 | 101.93 | 0.9105 | -41.0 | -80.7 | |
| 0.00 | 0.72 | 0.00 | 0.89 | -10.13 | 247.76 | -64.67 | 103.62 | 0.9172 | -393.0 | -368.8 | |
| 0.00 | 2.35 | 0.00 | 2.89 | -9.81 | 247.80 | -64.63 | 103.29 | 0.9165 | -661.0 | -507.5 | |
| 0.00 | 0.82 | 0.00 | 1.04 | -11.20 | 247.10 | -65.34 | 104.63 | 0.9230 | -390.0 | -379.0 | |
| 11.50 | -1.00 | 13.72 | -1.00 | -8.00 | 248.20 | -64.24 | 101.41 | 0.9115 | 175.0 | 999999 | |
| 5.89 | -1.00 | 7.39 | -1.00 | -9.68 | 247.19 | -65.24 | 103.03 | 0.9204 | -568.8 | 999999 | |
| 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. | |