| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 26.96 | 0.00 | 13.47 | 9.67 | 183.10 | -0.28 | 252.81 | 0.1022 | -447.0 | -484.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.58 | 5.17 | 189.62 | 6.25 | 252.06 | 0.1145 | -941.0 | -644.8 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 6.35 | 187.53 | 4.16 | 258.23 | 0.0739 | -811.0 | -626.6 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 6.08 | 187.23 | 3.85 | 253.52 | 0.0700 | -1179.0 | -962.6 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 12.38 | 186.50 | 3.12 | 329.40 | 0.1050 | -831.0 | -625.7 | |
| 0.00 | 1.70 | 0.00 | 0.84 | 11.53 | 186.27 | 2.89 | 326.65 | 0.0904 | -898.0 | -710.0 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 5.79 | 185.91 | 2.54 | 240.44 | 0.0509 | -930.0 | -695.0 | |
| 0.00 | 2.59 | 0.00 | 1.29 | 10.84 | 185.92 | 2.55 | 325.30 | 0.0771 | -858.0 | -803.3 | |
| 0.00 | 1.43 | 0.00 | 0.71 | 11.47 | 185.59 | 2.21 | 332.94 | 0.0836 | -883.0 | -629.7 | |
| 0.00 | 2.32 | 0.00 | 1.15 | 6.00 | 185.34 | 1.96 | 237.99 | 0.0404 | -1113.0 | -886.7 | |
| 0.00 | 3.93 | 0.00 | 1.95 | 11.08 | 185.34 | 1.96 | 333.43 | 0.0756 | -969.0 | -863.5 | |
| 0.00 | 1.70 | 0.00 | 0.84 | 6.00 | 185.16 | 1.78 | 235.43 | 0.0377 | -659.0 | -497.1 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 10.93 | 184.82 | 1.44 | 339.11 | 0.0695 | -894.0 | -715.1 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 11.30 | 184.76 | 1.38 | 341.59 | 0.0752 | -803.0 | -561.8 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 10.04 | 178.79 | -4.58 | 57.83 | 0.0934 | 947.0 | 762.8 | |
| 0.00 | 0.98 | 0.00 | 0.49 | 9.79 | 175.49 | -7.88 | 71.25 | 0.1434 | 514.0 | 456.5 | |
| 0.00 | 1.43 | 0.00 | 0.73 | 11.34 | 171.07 | -12.30 | 70.39 | 0.2228 | 725.0 | 585.8 | |
| 0.00 | 0.80 | 0.00 | 0.42 | 15.62 | 164.89 | -18.49 | 63.52 | 0.3427 | 736.0 | 581.2 | |
| 0.00 | 0.89 | 0.00 | 0.47 | 13.07 | 163.79 | -19.59 | 71.56 | 0.3458 | 801.0 | 549.1 | |
| 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. | |