| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.59 | 39.59 | 10.15 | 32.50 | -15.85 | 246.47 | -50.98 | 110.39 | 0.7992 | 268.6 | 59.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.72 | 6.97 | 2.16 | 5.53 | -16.03 | 248.13 | -49.33 | 111.08 | 0.7834 | 665.0 | 508.4 | |
| 0.00 | 1.90 | 0.00 | 1.52 | -15.78 | 247.87 | -49.58 | 110.69 | 0.7854 | 568.0 | 496.0 | |
| 0.00 | 1.72 | 0.00 | 1.37 | -15.56 | 247.75 | -49.71 | 110.38 | 0.7861 | 476.0 | 367.1 | |
| 0.45 | 1.27 | 0.36 | 1.02 | -15.88 | 247.40 | -50.06 | 110.67 | 0.7905 | 566.0 | 416.2 | |
| 4.98 | 6.43 | 4.00 | 5.16 | -15.50 | 247.43 | -50.03 | 110.21 | 0.7892 | 643.9 | 480.8 | |
| 0.00 | 0.91 | 0.00 | 0.74 | -16.23 | 246.82 | -50.63 | 110.95 | 0.7970 | 337.0 | 222.9 | |
| 0.00 | 0.27 | 0.00 | 0.22 | -15.66 | 246.92 | -50.53 | 110.27 | 0.7946 | 607.0 | 488.3 | |
| 4.44 | 7.15 | 3.63 | 5.85 | -15.66 | 246.62 | -50.84 | 110.19 | 0.7976 | 496.7 | 303.8 | |
| 0.00 | 1.00 | 0.00 | 0.81 | -15.28 | 246.50 | -50.96 | 109.70 | 0.7980 | 508.0 | 449.3 | |
| 0.00 | 1.36 | 0.00 | 1.12 | -15.44 | 246.24 | -51.21 | 109.82 | 0.8009 | 280.0 | 195.7 | |
| 0.00 | 0.91 | 0.00 | 0.75 | -14.68 | 246.10 | -51.36 | 108.86 | 0.8007 | 382.0 | 308.2 | |
| 0.00 | 2.99 | 0.00 | 2.54 | -16.15 | 244.96 | -52.50 | 110.35 | 0.8149 | -489.0 | -533.1 | |
| 0.00 | 0.82 | 0.00 | 0.69 | -15.51 | 245.14 | -52.32 | 109.63 | 0.8118 | -571.0 | -489.6 | |
| 0.00 | 1.54 | 0.00 | 1.32 | -16.28 | 244.59 | -52.87 | 110.41 | 0.8187 | -543.0 | -512.8 | |
| 0.00 | 1.99 | 0.00 | 1.72 | -16.41 | 244.28 | -53.18 | 110.48 | 0.8219 | -619.0 | -531.4 | |
| 0.00 | 1.36 | 0.00 | 1.21 | -16.48 | 243.22 | -54.24 | 110.31 | 0.8318 | -499.0 | -408.1 | |
| 0.00 | 1.00 | 0.00 | 0.93 | -16.97 | 241.50 | -55.96 | 110.48 | 0.8481 | -536.0 | -503.4 | |
| 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. | |