SOHO MDI 2000-11-02 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 110 | 0 | 63 | -27.28 | 290.76 | 4.53 | 187.59 | 0.5292 | 669.3 | 600.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 9 | 0 | 5 | -28.67 | 294.85 | 8.63 | 193.66 | 0.5596 | 913.0 | 687.9 | |
| 0 | 6 | 0 | 4 | -28.43 | 293.86 | 7.63 | 192.25 | 0.5530 | 761.0 | 701.0 | |
| 0 | 3 | 0 | 2 | -25.58 | 292.98 | 6.75 | 192.07 | 0.5092 | 717.0 | 644.8 | |
| 0 | 4 | 0 | 2 | -27.37 | 292.95 | 6.73 | 191.26 | 0.5352 | 836.0 | 731.4 | |
| 0 | 6 | 0 | 3 | -26.74 | 292.92 | 6.69 | 191.46 | 0.5260 | 619.0 | 628.8 | |
| 0 | 4 | 0 | 2 | -25.36 | 292.54 | 6.31 | 191.40 | 0.5045 | 594.0 | 612.3 | |
| 0 | 4 | 0 | 2 | -26.29 | 291.98 | 5.76 | 190.07 | 0.5167 | 734.0 | 664.2 | |
| 0 | 6 | 0 | 3 | -27.36 | 291.69 | 5.46 | 189.19 | 0.5317 | 750.0 | 694.8 | |
| 0 | 4 | 0 | 3 | -33.85 | 291.74 | 5.52 | 187.39 | 0.6232 | 579.0 | 476.1 | |
| 0 | 7 | 0 | 4 | -26.95 | 291.10 | 4.88 | 188.35 | 0.5244 | 970.0 | 791.1 | |
| 0 | 8 | 0 | 5 | -27.04 | 290.07 | 3.84 | 186.57 | 0.5236 | 1179.0 | 1025.6 | |
| 0 | 5 | 0 | 3 | -27.40 | 289.60 | 3.38 | 185.71 | 0.5282 | 787.0 | 826.0 | |
| 0 | 5 | 0 | 3 | -24.89 | 289.44 | 3.22 | 185.99 | 0.4905 | 887.0 | 767.2 | |
| 0 | 6 | 0 | 3 | -26.85 | 289.37 | 3.15 | 185.43 | 0.5198 | 1225.0 | 1011.8 | |
| 0 | 4 | 0 | 2 | -25.69 | 289.21 | 2.99 | 185.39 | 0.5022 | 544.0 | 317.0 | |
| 0 | 11 | 0 | 6 | -27.26 | 289.21 | 2.98 | 185.07 | 0.5256 | 878.0 | 730.6 | |
| 0 | 5 | 0 | 3 | -26.54 | 289.10 | 2.88 | 185.03 | 0.5148 | -191.0 | -72.2 | |
| 0 | 7 | 0 | 4 | -25.86 | 287.76 | 1.53 | 182.76 | 0.5032 | -811.0 | -689.8 | |
| 0 | 6 | 0 | 4 | -27.52 | 286.52 | 0.30 | 180.50 | 0.5276 | 746.0 | 682.6 | |
| 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. | |