SOHO MDI 2000-10-30 09:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24 | 148 | 17 | 102 | -28.18 | 292.90 | -29.35 | 140.85 | 0.6868 | 690.1 | 540.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -26.94 | 296.87 | -25.37 | 143.39 | 0.6430 | 679.0 | 616.8 | |
| 0 | 3 | 0 | 2 | -28.88 | 295.98 | -26.26 | 144.47 | 0.6691 | 693.0 | 582.4 | |
| 0 | 6 | 0 | 4 | -29.26 | 295.63 | -26.62 | 144.50 | 0.6754 | 497.0 | 540.2 | |
| 0 | 2 | 0 | 2 | -29.24 | 294.94 | -27.31 | 143.82 | 0.6804 | 568.0 | 449.5 | |
| 0 | 3 | 0 | 2 | -28.74 | 294.83 | -27.41 | 143.22 | 0.6765 | 537.0 | 581.2 | |
| 3 | 8 | 2 | 5 | -26.70 | 294.90 | -27.34 | 141.16 | 0.6566 | 762.5 | 718.2 | |
| 0 | 4 | 0 | 3 | -27.03 | 294.32 | -27.92 | 140.96 | 0.6645 | 521.0 | 580.1 | |
| 0 | 11 | 0 | 8 | -26.42 | 294.00 | -28.24 | 139.99 | 0.6615 | 914.0 | 719.5 | |
| 6 | 57 | 4 | 39 | -29.51 | 292.89 | -29.35 | 142.21 | 0.6984 | 966.3 | 526.1 | |
| 0 | 4 | 0 | 3 | -26.35 | 293.53 | -28.71 | 139.47 | 0.6648 | 695.0 | 582.3 | |
| 6 | -9 | 4 | -9 | -29.29 | 292.55 | -29.69 | 141.69 | 0.6991 | 677.5 | 999999 | |
| 0 | 2 | 0 | 1 | -29.72 | 292.42 | -29.82 | 141.99 | 0.7039 | 167.0 | 130.1 | |
| 0 | 7 | 0 | 5 | -27.90 | 292.94 | -29.31 | 140.59 | 0.6837 | 1012.0 | 712.6 | |
| 0 | 2 | 0 | 1 | -26.91 | 292.93 | -29.31 | 139.52 | 0.6749 | 489.0 | 497.7 | |
| 2 | 8 | 2 | 6 | -28.94 | 292.16 | -30.08 | 140.98 | 0.6991 | 594.6 | 562.0 | |
| 0 | 5 | 0 | 3 | -27.06 | 292.48 | -29.76 | 139.29 | 0.6800 | 817.0 | 767.7 | |
| 0 | 2 | 0 | 1 | -27.53 | 291.99 | -30.25 | 139.36 | 0.6882 | 567.0 | 477.5 | |
| 0 | 5 | 0 | 4 | -28.21 | 291.17 | -31.07 | 139.36 | 0.7007 | 366.0 | 281.6 | |
| 7 | 13 | 5 | 9 | -27.00 | 289.72 | -32.52 | 136.85 | 0.7028 | 581.4 | 496.0 | |
| 0 | 3 | 0 | 2 | -21.84 | 288.42 | -33.82 | 129.83 | 0.6751 | -496.0 | -369.1 | |
| 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. | |