| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.58 | 41.20 | 11.06 | 36.99 | 7.74 | 135.01 | 54.59 | 284.36 | 0.8350 | -32.3 | 362.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.73 | 11.66 | 8.62 | 11.52 | 7.28 | 138.73 | 58.31 | 282.79 | 0.8676 | -496.8 | -350.7 | |
| 0.00 | 1.12 | 0.00 | 1.03 | 7.11 | 135.98 | 55.57 | 283.31 | 0.8432 | -374.0 | -312.7 | |
| 0.00 | 0.60 | 0.00 | 0.54 | 6.61 | 135.26 | 54.84 | 282.93 | 0.8354 | -494.0 | -477.4 | |
| 0.00 | 0.95 | 0.00 | 0.86 | 8.21 | 135.41 | 54.99 | 284.75 | 0.8404 | 243.0 | 270.4 | |
| 0.00 | 0.60 | 0.00 | 0.54 | 6.14 | 134.87 | 54.45 | 282.48 | 0.8308 | -365.0 | -337.4 | |
| 0.00 | 0.78 | 0.00 | 0.70 | 7.65 | 135.03 | 54.61 | 284.21 | 0.8357 | 320.0 | 263.3 | |
| 0.00 | 1.04 | 0.00 | 0.92 | 7.44 | 134.73 | 54.31 | 284.04 | 0.8324 | 440.0 | 378.9 | |
| 0.00 | 0.35 | 0.00 | 0.30 | 6.72 | 134.35 | 53.93 | 283.32 | 0.8271 | 369.0 | 332.0 | |
| 0.52 | 2.07 | 0.45 | 1.82 | 7.21 | 134.28 | 53.86 | 283.90 | 0.8276 | 505.7 | 405.1 | |
| 0.00 | 0.78 | 0.00 | 0.67 | 8.70 | 133.30 | 52.88 | 285.96 | 0.8220 | 439.0 | 369.0 | |
| 0.00 | 0.60 | 0.00 | 0.52 | 7.78 | 133.07 | 52.65 | 284.95 | 0.8175 | 377.0 | 353.4 | |
| 1.12 | 19.61 | 0.96 | 16.70 | 8.22 | 132.86 | 52.44 | 285.53 | 0.8165 | 581.2 | 605.3 | |
| 1.21 | -12.00 | 1.03 | -12.00 | 8.17 | 132.65 | 52.23 | 285.54 | 0.8144 | 740.7 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.87 | 7.98 | 132.03 | 51.61 | 285.52 | 0.8078 | 560.0 | 476.1 | |
| 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. | |