| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.37 | 42.78 | 12.32 | 37.24 | -15.94 | 99.87 | -51.88 | 112.98 | 0.8234 | 372.0 | 230.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.36 | 15.07 | 6.20 | 12.71 | -15.84 | 101.21 | -50.55 | 113.33 | 0.8112 | 757.6 | 427.6 | |
| 0.00 | 1.21 | 0.00 | 1.03 | -15.48 | 100.84 | -50.92 | 112.78 | 0.8136 | 221.0 | 276.4 | |
| 0.00 | 1.82 | 0.00 | 1.55 | -15.68 | 100.72 | -51.04 | 112.97 | 0.8153 | 610.0 | 481.7 | |
| 0.00 | 0.26 | 0.00 | 0.22 | -15.44 | 100.61 | -51.15 | 112.64 | 0.8156 | 381.0 | 379.7 | |
| 6.58 | 12.64 | 5.67 | 10.92 | -15.90 | 100.19 | -51.56 | 113.04 | 0.8208 | 631.9 | 445.5 | |
| 0.00 | 2.34 | 0.00 | 2.02 | -15.19 | 100.00 | -51.76 | 112.14 | 0.8205 | 511.0 | 331.7 | |
| 0.00 | 0.69 | 0.00 | 0.60 | -15.36 | 99.89 | -51.87 | 112.30 | 0.8220 | 57.0 | 168.0 | |
| 0.00 | 0.43 | 0.00 | 0.37 | -14.57 | 99.96 | -51.80 | 111.40 | 0.8191 | 83.0 | 139.8 | |
| 0.00 | 1.30 | 0.00 | 1.15 | -15.87 | 99.19 | -52.56 | 112.66 | 0.8298 | 245.0 | 275.3 | |
| 0.00 | 1.30 | 0.00 | 1.16 | -15.89 | 98.88 | -52.88 | 112.58 | 0.8327 | -328.0 | -291.9 | |
| 0.00 | 1.13 | 0.00 | 1.03 | -16.18 | 97.82 | -53.93 | 112.56 | 0.8428 | 345.0 | 268.7 | |
| 0.00 | 1.91 | 0.00 | 1.77 | -15.54 | 97.07 | -54.69 | 111.58 | 0.8476 | -292.0 | -362.5 | |
| 0.43 | 1.47 | 0.45 | 1.52 | -19.08 | 94.10 | -57.66 | 114.61 | 0.8802 | -338.0 | -298.6 | |
| 0.00 | 1.21 | 0.00 | 1.19 | -16.54 | 95.32 | -56.44 | 112.18 | 0.8647 | -577.0 | -514.5 | |
| 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. | |