| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 124 | 711 | 90 | 512 | 4.83 | 72.10 | 45.47 | 282.15 | 0.7281 | -26.6 | -99.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20 | 261 | 15 | 201 | 3.63 | 75.98 | 49.35 | 279.45 | 0.7700 | 969.9 | 302.3 | |
| 26 | -1 | 20 | -1 | 4.51 | 75.76 | 49.13 | 280.63 | 0.7693 | 1089.3 | 999999 | |
| -2 | -1 | -2 | -1 | 4.07 | 75.60 | 48.97 | 280.11 | 0.7667 | 999999 | 999999 | |
| 0 | 11 | 0 | 8 | 4.49 | 74.48 | 47.84 | 280.94 | 0.7551 | 882.0 | 692.2 | |
| 9 | 20 | 7 | 15 | 4.67 | 73.69 | 47.06 | 281.38 | 0.7466 | 1000.5 | 763.5 | |
| 8 | 21 | 6 | 15 | 3.63 | 73.22 | 46.58 | 280.12 | 0.7388 | 837.5 | 717.3 | |
| 0 | 5 | 0 | 3 | 5.06 | 72.61 | 45.97 | 282.20 | 0.7351 | 450.0 | 483.3 | |
| 0 | 5 | 0 | 4 | 3.33 | 72.36 | 45.73 | 279.95 | 0.7281 | 402.0 | 455.2 | |
| 0 | 3 | 0 | 2 | 5.18 | 72.12 | 45.49 | 282.51 | 0.7298 | 506.0 | 547.5 | |
| 0 | 9 | 0 | 6 | 5.07 | 71.61 | 44.98 | 282.51 | 0.7236 | 866.0 | 645.4 | |
| 0 | 6 | 0 | 4 | 3.89 | 70.28 | 43.65 | 281.28 | 0.7046 | -555.0 | -400.2 | |
| 16 | 226 | 11 | 155 | 4.36 | 69.78 | 43.15 | 282.09 | 0.6998 | -809.5 | -536.5 | |
| 0 | 4 | 0 | 3 | 7.20 | 69.69 | 43.05 | 286.06 | 0.7072 | -460.0 | -381.2 | |
| 16 | -12 | 11 | -12 | 5.08 | 68.95 | 42.31 | 283.38 | 0.6917 | -1385.8 | 999999 | |
| 6 | -12 | 4 | -12 | 5.67 | 69.00 | 42.37 | 284.19 | 0.6941 | -972.0 | 999999 | |
| 0 | 6 | 0 | 4 | 6.15 | 68.68 | 42.05 | 284.98 | 0.6917 | -931.0 | -841.1 | |
| 23 | 134 | 16 | 92 | 6.76 | 68.38 | 41.74 | 285.95 | 0.6900 | -1437.2 | -634.1 | |
| 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. | |