| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66.68 | 423.89 | 40.78 | 258.70 | 31.33 | 188.18 | -7.94 | 11.66 | 0.5850 | -966.1 | -334.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.53 | 0.00 | 0.91 | 29.71 | 195.72 | -0.40 | 0.63 | 0.5498 | -695.0 | -520.9 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 29.25 | 195.52 | -0.60 | 0.97 | 0.5431 | -851.0 | -645.8 | |
| 0.00 | 1.70 | 0.00 | 1.00 | 29.49 | 195.48 | -0.64 | 1.02 | 0.5468 | -698.0 | -616.0 | |
| 0.00 | 0.93 | 0.00 | 0.56 | 30.06 | 194.12 | -2.00 | 3.13 | 0.5558 | -633.0 | -496.1 | |
| 0.00 | 1.70 | 0.00 | 1.13 | 37.99 | 189.56 | -6.55 | 7.74 | 0.6706 | 596.0 | 459.0 | |
| 0.00 | 1.44 | 0.00 | 0.88 | 31.80 | 189.98 | -6.14 | 8.95 | 0.5869 | -428.0 | -269.2 | |
| 61.42 | 402.33 | 37.39 | 245.22 | 31.24 | 188.17 | -7.95 | 11.73 | 0.5837 | -1279.1 | -347.8 | |
| 0.00 | 3.65 | 0.00 | 2.35 | 35.38 | 187.19 | -8.93 | 11.41 | 0.6420 | 780.0 | 691.2 | |
| 0.25 | -7.00 | 0.16 | -7.00 | 31.06 | 187.59 | -8.53 | 12.63 | 0.5830 | -972.0 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.86 | 28.88 | 186.38 | -9.74 | 15.48 | 0.5571 | -686.0 | -539.5 | |
| 5.01 | 5.86 | 3.23 | 3.78 | 34.88 | 184.91 | -11.21 | 14.43 | 0.6423 | 811.6 | 681.1 | |
| 0.00 | 0.76 | 0.00 | 0.47 | 31.88 | 185.26 | -10.86 | 15.47 | 0.6021 | -489.0 | -438.1 | |
| 0.00 | 1.19 | 0.00 | 0.74 | 31.93 | 184.34 | -11.78 | 16.68 | 0.6063 | -593.0 | -479.9 | |
| 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. | |