| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.07 | 175.01 | 43.83 | 109.50 | 33.99 | 267.77 | 7.45 | 349.85 | 0.6128 | 5.5 | -59.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.22 | 98.77 | 18.28 | 61.88 | 33.73 | 269.41 | 9.09 | 347.58 | 0.6131 | -1079.4 | -301.1 | |
| 2.29 | 3.82 | 1.44 | 2.40 | 34.43 | 268.22 | 7.90 | 349.41 | 0.6191 | -551.1 | -354.2 | |
| 0.00 | 1.19 | 0.00 | 0.75 | 34.69 | 268.10 | 7.78 | 349.66 | 0.6223 | -471.0 | -390.4 | |
| 0.00 | 0.59 | 0.00 | 0.37 | 34.54 | 267.87 | 7.55 | 349.91 | 0.6197 | -428.0 | -334.1 | |
| 0.00 | 1.19 | 0.00 | 0.73 | 33.09 | 267.07 | 6.74 | 350.50 | 0.5982 | 818.0 | 701.5 | |
| 0.00 | 1.10 | 0.00 | 0.68 | 32.95 | 266.95 | 6.63 | 350.61 | 0.5959 | 653.0 | 547.2 | |
| 0.00 | 1.10 | 0.00 | 0.69 | 34.38 | 266.81 | 6.49 | 351.25 | 0.6152 | -456.0 | -407.1 | |
| 2.29 | 6.37 | 1.42 | 3.94 | 33.35 | 266.69 | 6.37 | 351.09 | 0.6009 | 527.8 | 320.4 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 34.56 | 266.43 | 6.11 | 351.81 | 0.6169 | -237.0 | -246.5 | |
| 1.61 | -8.00 | 1.00 | -8.00 | 33.53 | 266.32 | 6.00 | 351.66 | 0.6026 | 450.7 | 999999 | |
| 5.10 | 5.69 | 3.21 | 3.59 | 34.97 | 265.44 | 5.12 | 353.20 | 0.6207 | 742.6 | 629.7 | |
| 0.00 | 1.53 | 0.00 | 0.95 | 33.60 | 265.33 | 5.00 | 353.04 | 0.6017 | 858.0 | 693.7 | |
| 28.37 | 49.00 | 17.73 | 30.57 | 34.37 | 265.19 | 4.87 | 353.40 | 0.6121 | 874.2 | 586.4 | |
| 1.19 | 3.14 | 0.75 | 1.99 | 35.23 | 265.13 | 4.81 | 353.67 | 0.6238 | 638.6 | 452.9 | |
| 0.00 | 0.25 | 0.00 | 0.16 | 35.53 | 265.04 | 4.72 | 353.85 | 0.6277 | 510.0 | 449.7 | |
| 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. | |