SOHO MDI 1999-12-11 12:47:33 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 186 | 1143 | 115 | 700 | 9.97 | 311.90 | 34.04 | 288.96 | 0.5802 | 248.4 | 147.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 113 | 654 | 73 | 426 | 9.55 | 317.23 | 39.37 | 285.38 | 0.6512 | 1294.0 | 570.7 | |
| 0 | 5 | 0 | 3 | 10.66 | 315.05 | 37.20 | 287.86 | 0.6266 | 868.0 | 687.5 | |
| 0 | 8 | 0 | 5 | 9.80 | 314.64 | 36.79 | 286.68 | 0.6183 | 1070.0 | 878.9 | |
| 0 | 8 | 0 | 5 | 9.38 | 314.54 | 36.69 | 286.04 | 0.6156 | 872.0 | 953.0 | |
| 0 | 3 | 0 | 2 | 8.79 | 314.42 | 36.57 | 285.15 | 0.6123 | 758.0 | 717.5 | |
| 0 | 7 | 0 | 4 | 6.13 | 314.06 | 36.21 | 280.92 | 0.6005 | 824.0 | 633.2 | |
| 0 | 11 | 0 | 7 | 9.26 | 314.19 | 36.33 | 285.98 | 0.6106 | 1087.0 | 987.7 | |
| 0 | 4 | 0 | 2 | 9.65 | 314.09 | 36.24 | 286.63 | 0.6105 | 785.0 | 815.0 | |
| 0 | 4 | 0 | 3 | 13.67 | 313.34 | 35.49 | 293.30 | 0.6165 | 659.0 | 590.8 | |
| 0 | 7 | 0 | 4 | 10.12 | 307.20 | 29.34 | 290.74 | 0.5180 | -686.0 | -617.0 | |
| 0 | 6 | 0 | 3 | 12.92 | 303.79 | 25.94 | 298.43 | 0.4868 | 557.0 | 453.5 | |
| 32 | 419 | 18 | 232 | 10.33 | 302.72 | 24.86 | 294.29 | 0.4557 | -1559.6 | -713.0 | |
| 7 | -12 | 4 | -12 | 10.41 | 301.87 | 24.01 | 295.16 | 0.4441 | -1650.9 | 999999 | |
| 26 | -12 | 15 | -12 | 11.34 | 301.69 | 23.84 | 297.25 | 0.4476 | -1606.1 | 999999 | |
| 8 | -12 | 5 | -12 | 10.80 | 301.64 | 23.79 | 296.17 | 0.4434 | -2031.8 | 999999 | |
| 0 | 7 | 0 | 4 | 9.71 | 301.56 | 23.70 | 293.95 | 0.4355 | -1028.0 | -845.6 | |
| 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. | |