| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.11 | 151.55 | 30.06 | 137.81 | -9.94 | 359.67 | -57.71 | 97.17 | 0.8412 | 558.8 | 323.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.69 | 0.00 | 0.60 | -9.41 | 1.60 | -55.77 | 96.45 | 0.8231 | -464.0 | -374.1 | |
| 0.00 | 1.47 | 0.00 | 1.26 | -5.81 | 2.21 | -55.17 | 92.02 | 0.8194 | 472.0 | 335.9 | |
| 16.51 | 125.19 | 14.91 | 112.56 | -10.35 | 359.97 | -57.41 | 97.66 | 0.8384 | 807.1 | 362.6 | |
| 12.97 | -3.00 | 11.65 | -3.00 | -9.56 | 0.19 | -57.19 | 96.70 | 0.8366 | 762.0 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.94 | -8.14 | 0.09 | -57.29 | 95.01 | 0.8383 | -176.0 | -269.2 | |
| 0.00 | 1.47 | 0.00 | 1.34 | -9.74 | 359.57 | -57.80 | 96.94 | 0.8423 | 377.0 | 272.2 | |
| 0.00 | 0.78 | 0.00 | 0.72 | -9.87 | 358.90 | -58.48 | 97.14 | 0.8485 | 278.0 | 274.7 | |
| 0.43 | 1.38 | 0.41 | 1.33 | -10.93 | 357.80 | -59.57 | 98.43 | 0.8579 | 338.0 | 275.5 | |
| 0.00 | 1.64 | 0.00 | 1.58 | -10.06 | 357.78 | -59.59 | 97.41 | 0.8584 | 466.0 | 353.1 | |
| 0.00 | 4.32 | 0.00 | 4.13 | -9.44 | 357.91 | -59.47 | 96.68 | 0.8576 | 568.0 | 458.6 | |
| 0.00 | 1.21 | 0.00 | 1.17 | -10.18 | 357.56 | -59.81 | 97.56 | 0.8603 | 387.0 | 371.7 | |
| 0.00 | 0.86 | 0.00 | 0.84 | -9.91 | 357.53 | -59.85 | 97.25 | 0.8607 | 20.0 | 33.1 | |
| 3.20 | 7.09 | 3.09 | 6.85 | -9.13 | 357.63 | -59.75 | 96.34 | 0.8602 | 492.0 | 195.3 | |
| 0.00 | 0.78 | 0.00 | 0.76 | -8.08 | 357.31 | -60.07 | 95.13 | 0.8636 | 315.0 | 292.6 | |
| 0.00 | 1.73 | 0.00 | 1.72 | -10.27 | 356.42 | -60.95 | 97.72 | 0.8701 | -486.0 | -466.5 | |
| 0.00 | 0.78 | 0.00 | 0.79 | -11.11 | 355.81 | -61.56 | 98.71 | 0.8749 | 306.0 | 265.8 | |
| 0.00 | 1.12 | 0.00 | 1.22 | -14.43 | 353.74 | -63.64 | 102.54 | 0.8909 | -349.0 | -341.8 | |
| 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. | |