SOHO MDI 2000-10-06 07:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53 | 400 | 38 | 288 | -21.82 | 316.51 | 37.02 | 230.90 | 0.7211 | -878.6 | -280.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18 | 272 | 13 | 200 | -21.71 | 318.69 | 39.20 | 232.67 | 0.7408 | -1035.3 | -396.7 | |
| 12 | -1 | 9 | -1 | -22.34 | 318.36 | 38.86 | 231.72 | 0.7416 | -755.7 | 999999 | |
| 14 | -1 | 10 | -1 | -21.74 | 318.01 | 38.51 | 232.17 | 0.7346 | -1196.0 | 999999 | |
| 3 | 34 | 2 | 24 | -20.49 | 315.64 | 36.14 | 231.97 | 0.7037 | -308.3 | -482.4 | |
| 0 | 4 | 0 | 3 | -20.37 | 315.14 | 35.65 | 231.75 | 0.6981 | 333.0 | 201.0 | |
| 0 | 7 | 0 | 5 | -23.25 | 315.15 | 35.66 | 228.40 | 0.7186 | -405.0 | -244.4 | |
| 6 | 24 | 4 | 16 | -21.33 | 312.72 | 33.22 | 228.70 | 0.6817 | -736.1 | -244.8 | |
| 0 | 6 | 0 | 4 | -21.20 | 312.09 | 32.59 | 228.33 | 0.6747 | -396.0 | -343.1 | |
| 0 | 10 | 0 | 7 | -23.55 | 311.66 | 32.17 | 225.26 | 0.6894 | -424.0 | -173.7 | |
| 0 | 4 | 0 | 3 | -24.59 | 311.10 | 31.60 | 223.63 | 0.6930 | 618.0 | 476.0 | |
| 0 | 6 | 0 | 4 | -21.26 | 310.24 | 30.75 | 226.66 | 0.6574 | 544.0 | 513.9 | |
| 0 | 5 | 0 | 3 | -20.94 | 309.25 | 29.76 | 226.13 | 0.6453 | 692.0 | 715.6 | |
| 0 | 10 | 0 | 7 | -21.90 | 309.18 | 29.68 | 224.94 | 0.6528 | 803.0 | 661.6 | |
| 0 | 12 | 0 | 8 | -22.09 | 307.98 | 28.48 | 223.56 | 0.6434 | 727.0 | 607.4 | |
| 0 | 6 | 0 | 4 | -23.20 | 304.77 | 25.27 | 219.02 | 0.6255 | 702.0 | 567.5 | |
| 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. | |