| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.96 | 260.49 | 45.83 | 267.16 | 11.88 | 262.17 | 58.44 | 287.78 | 0.8764 | -393.3 | -199.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.79 | 0.00 | 1.00 | 12.99 | 268.14 | 64.40 | 287.33 | 0.9223 | -260.0 | -230.0 | |
| 0.00 | 1.13 | 0.00 | 1.31 | 13.21 | 265.57 | 61.83 | 288.22 | 0.9054 | 259.0 | 233.2 | |
| 43.96 | 243.72 | 45.83 | 254.01 | 11.84 | 262.77 | 59.04 | 287.51 | 0.8820 | -641.9 | -237.8 | |
| 0.00 | 0.96 | 0.00 | 0.73 | 11.75 | 249.49 | 45.75 | 292.12 | 0.7594 | 373.0 | 310.7 | |
| 0.00 | 1.92 | 0.00 | 1.46 | 12.89 | 249.17 | 45.44 | 293.67 | 0.7606 | 536.0 | 394.8 | |
| 0.00 | 1.05 | 0.00 | 0.78 | 11.82 | 248.50 | 44.77 | 292.65 | 0.7492 | 592.0 | 458.4 | |
| 0.00 | 1.40 | 0.00 | 1.02 | 11.05 | 247.96 | 44.22 | 291.94 | 0.7403 | 466.0 | 358.4 | |
| 0.00 | 1.40 | 0.00 | 1.05 | 13.13 | 248.36 | 44.63 | 294.35 | 0.7532 | 563.0 | 469.8 | |
| 0.00 | 0.79 | 0.00 | 0.58 | 12.94 | 248.02 | 44.28 | 294.28 | 0.7488 | 598.0 | 549.6 | |
| 0.00 | 2.62 | 0.00 | 1.94 | 12.92 | 247.80 | 44.06 | 294.37 | 0.7464 | 740.0 | 596.9 | |
| 0.00 | 0.61 | 0.00 | 0.45 | 13.57 | 247.60 | 43.87 | 295.27 | 0.7472 | 429.0 | 380.0 | |
| 0.00 | 1.05 | 0.00 | 0.77 | 13.55 | 247.39 | 43.65 | 295.35 | 0.7449 | 640.0 | 546.7 | |
| 0.00 | 2.18 | 0.00 | 1.48 | 12.05 | 242.54 | 38.81 | 296.06 | 0.6846 | 652.0 | 535.2 | |
| 0.00 | 0.87 | 0.00 | 0.58 | 11.38 | 242.00 | 38.27 | 295.47 | 0.6748 | 691.0 | 607.2 | |
| 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. | |