| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.66 | 301.40 | 25.84 | 166.34 | 5.80 | 45.53 | -23.77 | 83.65 | 0.4400 | -1092.8 | -412.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.66 | 12.39 | 74.95 | 5.65 | 341.21 | 0.2999 | -920.0 | -641.1 | |
| 0.00 | 1.87 | 0.00 | 0.95 | 9.71 | 66.04 | -3.27 | 13.30 | 0.2452 | -1038.0 | -835.7 | |
| 0.00 | 1.10 | 0.00 | 0.56 | 8.80 | 65.99 | -3.32 | 14.44 | 0.2304 | -736.0 | -640.7 | |
| 0.00 | 4.16 | 0.00 | 2.13 | 9.74 | 65.68 | -3.62 | 14.67 | 0.2472 | -935.0 | -772.8 | |
| 0.00 | 0.93 | 0.00 | 0.48 | 8.12 | 63.69 | -5.61 | 24.72 | 0.2326 | -857.0 | -670.1 | |
| 0.00 | 1.61 | 0.00 | 0.84 | 10.39 | 60.40 | -8.91 | 31.51 | 0.2927 | -788.0 | -688.2 | |
| 0.00 | 3.48 | 0.00 | 1.80 | 10.25 | 60.16 | -9.15 | 32.47 | 0.2927 | -643.0 | -731.2 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 12.49 | 59.41 | -9.89 | 30.61 | 0.3308 | -658.0 | -545.7 | |
| 0.00 | 0.34 | 0.00 | 0.18 | 5.94 | 55.56 | -13.74 | 54.04 | 0.2932 | -394.0 | -605.0 | |
| 0.00 | 2.12 | 0.00 | 1.13 | 9.52 | 52.88 | -16.43 | 50.29 | 0.3642 | -766.0 | -687.6 | |
| 0.00 | 0.93 | 0.00 | 0.51 | 13.66 | 51.29 | -18.01 | 44.98 | 0.4269 | -802.0 | -640.2 | |
| 0.00 | 1.61 | 0.00 | 0.88 | 11.11 | 49.95 | -19.36 | 51.63 | 0.4166 | -798.0 | -618.2 | |
| 0.00 | 1.70 | 0.00 | 0.94 | 12.56 | 48.52 | -20.78 | 50.93 | 0.4480 | -649.0 | -547.5 | |
| 0.00 | 1.19 | 0.00 | 0.66 | 12.16 | 48.27 | -21.04 | 51.97 | 0.4474 | -791.0 | -674.2 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 4.48 | 47.96 | -21.35 | 68.46 | 0.3919 | -895.0 | -744.7 | |
| 46.66 | 274.59 | 25.84 | 152.16 | 5.50 | 44.44 | -24.86 | 69.16 | 0.4497 | -1409.9 | -391.2 | |
| 0.00 | 0.68 | 0.00 | 0.38 | -0.03 | 42.86 | -26.45 | 82.00 | 0.4516 | 678.0 | 554.4 | |
| 0.00 | 1.36 | 0.00 | 0.77 | -6.96 | 40.21 | -29.09 | 97.06 | 0.4883 | 608.0 | 389.3 | |
| 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. | |