SOHO MDI 1999-04-10 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57 | 284 | 36 | 181 | -18.18 | 233.07 | -38.30 | 111.54 | 0.6349 | -218.4 | 134.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 8 | 0 | 5 | -16.76 | 237.06 | -34.31 | 110.71 | 0.5793 | -1277.0 | -928.8 | |
| 0 | 4 | 0 | 2 | -18.47 | 236.13 | -35.24 | 113.15 | 0.5974 | 622.0 | 322.4 | |
| 0 | 5 | 0 | 3 | -17.55 | 236.20 | -35.18 | 111.68 | 0.5934 | -916.0 | -705.4 | |
| 23 | 105 | 14 | 65 | -17.60 | 235.63 | -35.74 | 111.54 | 0.6008 | -1340.7 | -587.6 | |
| -4 | -4 | -4 | -4 | -17.34 | 235.44 | -35.94 | 111.05 | 0.6025 | 999999 | 999999 | |
| 10 | -4 | 6 | -4 | -17.35 | 234.93 | -36.45 | 110.88 | 0.6092 | -924.6 | 999999 | |
| 0 | 3 | 0 | 2 | -16.98 | 233.99 | -37.38 | 109.96 | 0.6201 | -315.0 | -308.8 | |
| 0 | 3 | 0 | 2 | -17.84 | 233.73 | -37.64 | 111.23 | 0.6260 | -351.0 | -193.2 | |
| 0 | 3 | 0 | 2 | -18.18 | 233.39 | -37.99 | 111.64 | 0.6314 | -270.0 | -124.7 | |
| 3 | 23 | 2 | 15 | -19.65 | 232.40 | -38.97 | 113.53 | 0.6483 | 803.3 | 747.8 | |
| 0 | 4 | 0 | 2 | -18.65 | 232.53 | -38.85 | 112.06 | 0.6436 | 558.0 | 515.0 | |
| 4 | 120 | 3 | 79 | -18.98 | 232.01 | -39.36 | 112.38 | 0.6510 | 789.8 | 613.8 | |
| 14 | -12 | 9 | -12 | -18.45 | 230.70 | -40.67 | 111.18 | 0.6653 | 1158.7 | 999999 | |
| 3 | -12 | 2 | -12 | -19.16 | 230.49 | -40.88 | 112.16 | 0.6698 | 770.3 | 999999 | |
| 0 | 6 | 0 | 4 | -17.81 | 230.78 | -40.60 | 110.26 | 0.6627 | 710.0 | 649.2 | |
| 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. | |