SOHO MDI 2000-11-03 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5 | 114 | 3 | 74 | -27.53 | 290.31 | 26.92 | 217.80 | 0.6566 | 530.6 | 351.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | -24.25 | 296.42 | 33.04 | 227.03 | 0.6817 | 643.0 | 512.2 | |
| 0 | 5 | 0 | 4 | -27.40 | 293.34 | 29.96 | 220.85 | 0.6802 | 584.0 | 561.4 | |
| 0 | 1 | 0 | 1 | -26.19 | 291.86 | 28.48 | 220.83 | 0.6568 | 650.0 | 692.4 | |
| 0 | 4 | 0 | 3 | -27.27 | 292.06 | 28.68 | 219.83 | 0.6683 | 600.0 | 569.1 | |
| 0 | 5 | 0 | 3 | -26.97 | 291.34 | 27.95 | 219.47 | 0.6595 | 702.0 | 662.4 | |
| 0 | 6 | 0 | 4 | -28.64 | 291.21 | 27.83 | 217.59 | 0.6740 | 525.0 | 310.7 | |
| 5 | 12 | 3 | 8 | -27.90 | 290.96 | 27.57 | 218.11 | 0.6651 | 652.0 | 387.6 | |
| 0 | 4 | 0 | 3 | -27.17 | 290.71 | 27.32 | 218.65 | 0.6562 | 769.0 | 731.3 | |
| 0 | 6 | 0 | 4 | -28.53 | 290.64 | 27.25 | 217.16 | 0.6685 | -562.0 | -576.5 | |
| 0 | 5 | 0 | 3 | -27.11 | 290.06 | 26.67 | 218.08 | 0.6502 | 915.0 | 795.5 | |
| 0 | 5 | 0 | 3 | -29.07 | 290.60 | 27.21 | 216.56 | 0.6733 | -552.0 | -568.4 | |
| 0 | 5 | 0 | 3 | -27.64 | 289.96 | 26.57 | 217.41 | 0.6546 | 647.0 | 550.3 | |
| 0 | 27 | 0 | 17 | -27.85 | 289.48 | 26.09 | 216.71 | 0.6528 | 722.0 | 477.6 | |
| 0 | 7 | 0 | 5 | -29.46 | 289.66 | 26.28 | 215.28 | 0.6699 | -754.0 | -521.5 | |
| 0 | 12 | 0 | 7 | -26.80 | 288.92 | 25.54 | 217.26 | 0.6380 | 774.0 | 669.9 | |
| 0 | 5 | 0 | 3 | -24.32 | 282.34 | 18.96 | 212.16 | 0.5584 | 474.0 | 361.4 | |
| 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. | |