| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.50 | 338.29 | 44.35 | 276.41 | 11.93 | 261.94 | 49.41 | 290.94 | 0.7964 | -556.4 | -274.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.44 | 0.00 | 0.38 | 10.95 | 265.69 | 53.16 | 288.32 | 0.8298 | -193.0 | -202.0 | |
| 0.00 | 0.70 | 0.00 | 0.62 | 13.03 | 265.52 | 52.99 | 290.77 | 0.8342 | 332.0 | 284.4 | |
| 53.50 | 317.07 | 44.35 | 262.46 | 11.87 | 262.67 | 50.14 | 290.47 | 0.8040 | -959.5 | -318.3 | |
| 0.00 | 0.96 | 0.00 | 0.72 | 16.00 | 255.69 | 43.16 | 298.62 | 0.7514 | -581.0 | -473.4 | |
| 0.00 | 2.36 | 0.00 | 1.55 | 11.43 | 249.53 | 37.00 | 296.33 | 0.6605 | 548.0 | 478.7 | |
| 0.00 | 2.62 | 0.00 | 1.72 | 11.62 | 249.52 | 36.99 | 296.59 | 0.6615 | 456.0 | 355.2 | |
| 0.00 | 0.35 | 0.00 | 0.23 | 12.62 | 249.42 | 36.89 | 298.02 | 0.6659 | 618.0 | 578.8 | |
| 0.00 | 0.96 | 0.00 | 0.63 | 12.88 | 248.66 | 36.13 | 298.87 | 0.6587 | 636.0 | 482.0 | |
| 0.00 | 1.13 | 0.00 | 0.74 | 12.01 | 248.37 | 35.84 | 297.87 | 0.6502 | 633.0 | 493.7 | |
| 0.00 | 1.31 | 0.00 | 0.83 | 10.42 | 247.61 | 35.08 | 296.13 | 0.6320 | 654.0 | 500.9 | |
| 0.00 | 1.05 | 0.00 | 0.67 | 11.26 | 247.17 | 34.64 | 297.64 | 0.6316 | 679.0 | 497.4 | |
| 0.00 | 0.96 | 0.00 | 0.62 | 13.28 | 247.18 | 34.65 | 300.45 | 0.6443 | 587.0 | 479.2 | |
| 0.00 | 0.70 | 0.00 | 0.45 | 13.33 | 246.11 | 33.58 | 301.31 | 0.6323 | 607.0 | 507.8 | |
| 0.00 | 0.96 | 0.00 | 0.61 | 15.28 | 244.16 | 31.63 | 305.54 | 0.6240 | 646.0 | 502.1 | |
| 0.00 | 3.40 | 0.00 | 2.17 | 16.53 | 244.13 | 31.60 | 307.23 | 0.6332 | 645.0 | 514.8 | |
| 0.00 | 1.05 | 0.00 | 0.67 | 16.85 | 243.57 | 31.04 | 308.14 | 0.6297 | 595.0 | 492.0 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 10.23 | 242.47 | 29.94 | 299.68 | 0.5675 | 838.0 | 668.9 | |
| 0.00 | 1.22 | 0.00 | 0.71 | 10.70 | 239.37 | 26.84 | 303.26 | 0.5326 | 716.0 | 574.5 | |
| 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. | |