| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.31 | 253.88 | 14.51 | 134.96 | 16.84 | 168.80 | 17.62 | 306.68 | 0.3636 | -475.9 | -368.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.83 | 13.36 | 173.34 | 22.17 | 293.23 | 0.4012 | -804.0 | -691.8 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 17.05 | 171.40 | 20.22 | 303.63 | 0.3985 | -694.0 | -586.6 | |
| 17.69 | 232.30 | 9.41 | 123.54 | 16.63 | 169.26 | 18.08 | 305.45 | 0.3667 | -1341.7 | -451.4 | |
| 5.08 | -3.00 | 2.70 | -3.00 | 16.36 | 169.00 | 17.82 | 305.17 | 0.3609 | -1464.2 | 999999 | |
| 0.82 | -3.00 | 0.43 | -3.00 | 16.99 | 168.93 | 17.75 | 306.73 | 0.3654 | -759.1 | 999999 | |
| 3.72 | -3.00 | 1.97 | -3.00 | 16.62 | 168.76 | 17.58 | 306.12 | 0.3599 | -1328.9 | 999999 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 15.95 | 166.71 | 15.54 | 307.69 | 0.3269 | -864.0 | -570.4 | |
| 0.00 | 1.63 | 0.00 | 0.86 | 18.20 | 166.31 | 15.13 | 313.73 | 0.3447 | 880.0 | 598.9 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 20.54 | 166.26 | 15.09 | 318.61 | 0.3703 | 751.0 | 600.7 | |
| 0.00 | 2.81 | 0.00 | 1.51 | 21.55 | 166.34 | 15.16 | 320.36 | 0.3829 | 945.0 | 520.3 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 18.99 | 164.42 | 13.24 | 319.09 | 0.3322 | 989.0 | 720.9 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 22.13 | 164.30 | 13.12 | 325.21 | 0.3701 | 814.0 | 528.3 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 18.31 | 163.97 | 12.79 | 318.58 | 0.3192 | 831.0 | 581.2 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 22.87 | 164.20 | 13.02 | 326.60 | 0.3788 | 877.0 | 702.2 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 17.61 | 162.74 | 11.57 | 319.79 | 0.2973 | 1023.0 | 748.7 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 23.22 | 162.81 | 11.63 | 329.95 | 0.3715 | 867.0 | 654.9 | |
| 0.00 | 3.54 | 0.00 | 1.84 | 20.44 | 160.37 | 9.19 | 331.31 | 0.3130 | 1099.0 | 858.6 | |
| 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. | |