SOHO MDI 2000-11-03 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 134 | 10 | 89 | -27.60 | 290.17 | 28.54 | 219.32 | 0.6703 | 564.0 | 260.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 3 | -24.12 | 296.41 | 34.78 | 228.56 | 0.6969 | 82.0 | 104.5 | |
| 0 | 3 | 0 | 2 | -27.40 | 293.46 | 31.83 | 222.47 | 0.6958 | 503.0 | 503.4 | |
| 0 | 5 | 0 | 3 | -26.18 | 291.87 | 30.25 | 222.47 | 0.6719 | 730.0 | 530.4 | |
| 0 | 4 | 0 | 3 | -27.25 | 291.94 | 30.31 | 221.34 | 0.6817 | 658.0 | 561.2 | |
| 0 | 4 | 0 | 3 | -26.96 | 291.30 | 29.68 | 221.09 | 0.6738 | 751.0 | 676.2 | |
| 3 | 9 | 2 | 6 | -27.98 | 290.96 | 29.33 | 219.68 | 0.6799 | 491.9 | 391.6 | |
| 0 | 11 | 0 | 8 | -28.67 | 291.12 | 29.49 | 219.09 | 0.6873 | 100.0 | -101.4 | |
| 0 | 5 | 0 | 3 | -27.16 | 290.67 | 29.04 | 220.29 | 0.6702 | 839.0 | 754.4 | |
| 0 | 6 | 0 | 4 | -27.05 | 290.04 | 28.41 | 219.84 | 0.6639 | 911.0 | 811.8 | |
| 0 | 3 | 0 | 2 | -29.15 | 290.66 | 29.03 | 218.18 | 0.6880 | -789.0 | -727.6 | |
| 0 | 12 | 0 | 8 | -27.35 | 289.73 | 28.10 | 219.22 | 0.6641 | 981.0 | 777.9 | |
| 0 | 8 | 0 | 5 | -29.04 | 290.02 | 28.40 | 217.72 | 0.6820 | -1025.0 | -838.2 | |
| 13 | 43 | 8 | 28 | -27.92 | 289.30 | 27.67 | 218.20 | 0.6659 | 671.8 | 225.7 | |
| 0 | 9 | 0 | 6 | -26.74 | 288.98 | 27.35 | 219.15 | 0.6522 | 653.0 | 566.7 | |
| 0 | 5 | 0 | 3 | -29.39 | 289.58 | 27.95 | 216.95 | 0.6818 | -532.0 | -485.7 | |
| 0 | 3 | 0 | 2 | -24.29 | 282.28 | 20.66 | 214.40 | 0.5713 | 442.0 | 340.7 | |
| 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. | |