SOHO MDI 2000-11-05 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 127 | 0 | 71 | 10.26 | 267.04 | 28.25 | 285.28 | 0.4835 | 160.7 | 74.5 | |
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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 | 7.23 | 276.11 | 37.32 | 276.95 | 0.6082 | 816.0 | 722.2 | |
| 0 | 5 | 0 | 3 | 6.25 | 275.39 | 36.60 | 275.38 | 0.5976 | 797.0 | 653.6 | |
| 0 | 4 | 0 | 2 | 8.62 | 274.08 | 35.29 | 279.55 | 0.5815 | 542.0 | 564.3 | |
| 0 | 4 | 0 | 2 | 10.74 | 273.38 | 34.59 | 283.35 | 0.5755 | 547.0 | 523.2 | |
| 0 | 10 | 0 | 6 | 9.32 | 271.98 | 33.19 | 281.19 | 0.5529 | 896.0 | 648.8 | |
| 0 | 5 | 0 | 3 | 10.00 | 271.36 | 32.57 | 282.57 | 0.5454 | 721.0 | 649.1 | |
| 0 | 8 | 0 | 5 | 8.98 | 269.46 | 30.68 | 281.16 | 0.5158 | -266.0 | 98.4 | |
| 0 | 5 | 0 | 3 | 10.33 | 269.51 | 30.72 | 283.75 | 0.5195 | 717.0 | 613.2 | |
| 0 | 9 | 0 | 5 | 9.60 | 269.39 | 30.60 | 282.38 | 0.5160 | 1239.0 | 1039.1 | |
| 0 | 5 | 0 | 3 | 9.31 | 268.73 | 29.94 | 282.02 | 0.5056 | 480.0 | 337.0 | |
| 0 | 5 | 0 | 3 | 8.89 | 267.53 | 28.74 | 281.51 | 0.4868 | 583.0 | 436.1 | |
| 0 | 4 | 0 | 2 | 11.64 | 267.31 | 28.52 | 287.16 | 0.4915 | 523.0 | 413.6 | |
| 0 | 5 | 0 | 3 | 11.54 | 266.98 | 28.20 | 287.10 | 0.4864 | 450.0 | 503.0 | |
| 0 | 9 | 0 | 5 | 11.13 | 265.17 | 26.39 | 287.12 | 0.4582 | -666.0 | -536.9 | |
| 0 | 4 | 0 | 2 | 12.33 | 265.21 | 26.42 | 289.64 | 0.4635 | -546.0 | -533.0 | |
| 0 | 4 | 0 | 2 | 7.72 | 263.82 | 25.03 | 280.09 | 0.4277 | -542.0 | -402.8 | |
| 0 | 26 | 0 | 14 | 12.16 | 261.43 | 22.64 | 291.79 | 0.4070 | -989.0 | -721.4 | |
| 0 | 4 | 0 | 2 | 10.34 | 261.19 | 22.40 | 287.59 | 0.3950 | -729.0 | -634.2 | |
| 0 | 4 | 0 | 2 | 11.05 | 259.14 | 20.35 | 290.89 | 0.3670 | -734.0 | -658.0 | |
| 0 | 4 | 0 | 2 | 12.77 | 254.50 | 15.71 | 300.96 | 0.3094 | -624.0 | -537.7 | |
| 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. | |