| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.08 | 0.00 | 12.75 | 18.00 | 359.19 | -4.56 | 302.85 | 0.2161 | -461.6 | -467.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 5.03 | 0.00 | 2.51 | 14.50 | 4.51 | 0.76 | 354.31 | 0.1307 | -866.0 | -742.5 | |
| 0.00 | 1.44 | 0.00 | 0.73 | 19.64 | 2.57 | -1.18 | 5.08 | 0.2196 | -832.0 | -676.6 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 17.75 | 1.82 | -1.93 | 9.80 | 0.1891 | -1123.0 | -942.4 | |
| 0.00 | 1.71 | 0.00 | 0.87 | 20.10 | 1.41 | -2.34 | 9.65 | 0.2299 | -886.0 | -681.1 | |
| 0.00 | 0.72 | 0.00 | 0.37 | 20.13 | 0.57 | -3.18 | 12.98 | 0.2332 | -806.0 | -598.1 | |
| 0.00 | 3.95 | 0.00 | 2.01 | 19.72 | 0.22 | -3.53 | 14.80 | 0.2279 | -1121.0 | -839.7 | |
| 0.00 | 1.89 | 0.00 | 0.95 | 16.97 | 0.24 | -3.51 | 18.75 | 0.1827 | -997.0 | -771.2 | |
| 0.00 | 1.89 | 0.00 | 0.96 | 19.56 | 359.93 | -3.82 | 16.14 | 0.2266 | -1044.0 | -803.5 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 17.59 | 359.91 | -3.84 | 19.23 | 0.1945 | -744.0 | -645.2 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 15.52 | 358.82 | -4.93 | 29.32 | 0.1698 | -959.0 | -721.5 | |
| 0.00 | 2.42 | 0.00 | 1.24 | 17.69 | 354.24 | -9.51 | 40.23 | 0.2447 | 894.0 | 732.4 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 22.87 | 347.29 | -16.46 | 43.30 | 0.3823 | 821.0 | 696.4 | |
| 0.00 | 0.36 | 0.00 | 0.19 | 20.40 | 346.50 | -17.25 | 49.70 | 0.3660 | 578.0 | 670.2 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 17.79 | 345.54 | -18.21 | 57.18 | 0.3555 | 623.0 | 524.8 | |
| 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. | |