| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.45 | 156.71 | 18.47 | 127.51 | 20.17 | 194.03 | 49.76 | 295.26 | 0.7942 | -484.0 | -238.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.06 | 136.83 | 5.06 | 112.78 | 20.09 | 195.37 | 51.10 | 294.69 | 0.8067 | -575.6 | -269.2 | |
| 16.39 | -1.00 | 13.41 | -1.00 | 19.85 | 194.57 | 50.30 | 294.63 | 0.7984 | -935.9 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.66 | 17.10 | 192.30 | 48.03 | 291.91 | 0.7683 | -505.0 | -396.7 | |
| 0.00 | 0.77 | 0.00 | 0.60 | 20.66 | 191.59 | 47.32 | 296.61 | 0.7717 | -471.0 | -412.4 | |
| 0.00 | 2.39 | 0.00 | 1.74 | 15.71 | 189.61 | 45.33 | 290.94 | 0.7354 | -668.0 | -558.1 | |
| 0.00 | 1.88 | 0.00 | 1.45 | 21.08 | 191.11 | 46.84 | 297.30 | 0.7683 | -660.0 | -532.2 | |
| 0.00 | 2.99 | 0.00 | 2.31 | 21.42 | 191.16 | 46.89 | 297.72 | 0.7700 | -605.0 | -572.3 | |
| 0.00 | 0.77 | 0.00 | 0.59 | 22.12 | 190.95 | 46.68 | 298.66 | 0.7704 | -520.0 | -486.3 | |
| 0.00 | 1.62 | 0.00 | 1.21 | 20.36 | 189.77 | 45.50 | 296.91 | 0.7523 | 392.0 | 328.2 | |
| 0.00 | 0.94 | 0.00 | 0.67 | 23.44 | 185.84 | 41.57 | 302.58 | 0.7248 | 643.0 | 541.7 | |
| 0.00 | 0.94 | 0.00 | 0.68 | 24.41 | 185.79 | 41.52 | 303.83 | 0.7290 | 298.0 | 306.2 | |
| 0.00 | 1.02 | 0.00 | 0.74 | 25.22 | 185.95 | 41.68 | 304.75 | 0.7345 | 430.0 | 338.1 | |
| 0.00 | 0.85 | 0.00 | 0.59 | 21.00 | 184.17 | 39.90 | 300.25 | 0.6956 | 460.0 | 344.7 | |
| 0.00 | 4.01 | 0.00 | 2.90 | 27.07 | 184.51 | 40.24 | 307.81 | 0.7304 | 696.0 | 517.6 | |
| 0.00 | 0.85 | 0.00 | 0.59 | 26.59 | 181.71 | 37.44 | 308.89 | 0.7008 | 742.0 | 559.7 | |
| 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. | |