| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.71 | 29.37 | 2.47 | 19.39 | 9.12 | 289.45 | 41.48 | 275.81 | 0.6601 | -275.3 | -294.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.03 | 0.00 | 1.52 | 12.84 | 296.97 | 49.00 | 281.03 | 0.7520 | -193.0 | -232.8 | |
| 0.80 | 3.54 | 0.55 | 2.47 | 5.16 | 292.94 | 44.98 | 270.35 | 0.7063 | -639.2 | -493.3 | |
| 0.35 | 1.33 | 0.25 | 0.92 | 5.30 | 292.70 | 44.74 | 270.52 | 0.7032 | -686.8 | -577.9 | |
| 0.00 | 1.33 | 0.00 | 0.91 | 7.92 | 292.45 | 44.49 | 274.25 | 0.6983 | -735.0 | -570.9 | |
| 0.00 | 1.59 | 0.00 | 1.10 | 10.00 | 292.56 | 44.60 | 277.24 | 0.6994 | -666.0 | -594.5 | |
| 0.00 | 1.33 | 0.00 | 0.88 | 13.00 | 290.14 | 42.17 | 281.76 | 0.6705 | -316.0 | -347.6 | |
| 0.00 | 1.33 | 0.00 | 0.86 | 6.98 | 288.53 | 40.57 | 272.62 | 0.6485 | 554.0 | 379.1 | |
| 2.56 | 5.04 | 1.67 | 3.29 | 10.94 | 288.96 | 41.00 | 278.73 | 0.6539 | -855.6 | -662.7 | |
| 0.00 | 0.71 | 0.00 | 0.46 | 8.30 | 288.57 | 40.61 | 274.68 | 0.6485 | 584.0 | 488.9 | |
| 0.00 | 2.56 | 0.00 | 1.65 | 11.95 | 288.00 | 40.04 | 280.37 | 0.6421 | -796.0 | -615.2 | |
| 0.00 | 0.80 | 0.00 | 0.51 | 12.06 | 287.82 | 39.86 | 280.55 | 0.6398 | -581.0 | -555.1 | |
| 0.00 | 1.15 | 0.00 | 0.73 | 2.59 | 286.69 | 38.73 | 265.50 | 0.6292 | 581.0 | 448.5 | |
| 0.00 | 0.62 | 0.00 | 0.40 | 12.58 | 287.68 | 39.71 | 281.40 | 0.6384 | -496.0 | -474.7 | |
| 0.00 | 0.88 | 0.00 | 0.57 | 12.69 | 287.50 | 39.53 | 281.58 | 0.6362 | -574.0 | -498.8 | |
| 0.00 | 1.24 | 0.00 | 0.79 | 17.06 | 286.36 | 38.40 | 288.69 | 0.6291 | -202.0 | -304.2 | |
| 0.00 | 1.77 | 0.00 | 1.09 | 6.43 | 284.56 | 36.60 | 271.44 | 0.5948 | 382.0 | 256.5 | |
| 0.00 | 1.15 | 0.00 | 0.70 | 4.38 | 284.19 | 36.22 | 267.93 | 0.5918 | 656.0 | 524.3 | |
| 0.00 | 0.97 | 0.00 | 0.54 | 1.31 | 273.60 | 25.63 | 258.73 | 0.4428 | -643.0 | -482.1 | |
| 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. | |