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 |
| 86 | 469 | 64 | 353 | -23.29 | 305.17 | 41.79 | 234.12 | 0.7572 | -600.9 | -263.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 67 | 13 | 52 | -22.45 | 307.78 | 44.40 | 236.57 | 0.7772 | -862.3 | -408.8 | |
| -1 | -1 | -1 | -1 | -22.60 | 307.44 | 44.05 | 236.21 | 0.7747 | 999999 | 999999 | |
| 0 | 6 | 0 | 4 | -22.93 | 306.30 | 42.91 | 235.21 | 0.7659 | -535.0 | -378.6 | |
| 0 | 19 | 0 | 14 | -22.43 | 305.76 | 42.38 | 235.50 | 0.7584 | -774.0 | -609.6 | |
| 7 | 14 | 5 | 10 | -20.32 | 304.96 | 41.57 | 237.58 | 0.7396 | -661.7 | -542.2 | |
| 32 | 245 | 24 | 188 | -24.08 | 306.02 | 42.63 | 233.73 | 0.7694 | -944.2 | -297.7 | |
| 4 | -6 | 3 | -6 | -23.61 | 305.31 | 41.93 | 233.87 | 0.7605 | -963.5 | 999999 | |
| -6 | -6 | -6 | -6 | -24.32 | 305.60 | 42.22 | 233.21 | 0.7669 | 999999 | 999999 | |
| 4 | 14 | 3 | 11 | -22.37 | 304.62 | 41.24 | 234.91 | 0.7473 | -369.6 | -409.0 | |
| 5 | 12 | 4 | 9 | -23.26 | 304.39 | 41.01 | 233.73 | 0.7501 | -843.9 | -685.7 | |
| 4 | 18 | 3 | 13 | -22.19 | 303.51 | 40.13 | 234.47 | 0.7357 | 629.2 | 180.9 | |
| 4 | 18 | 3 | 13 | -21.05 | 302.70 | 39.32 | 235.35 | 0.7212 | -612.5 | -462.1 | |
| 0 | 7 | 0 | 5 | -25.52 | 304.22 | 40.83 | 231.03 | 0.7613 | 548.0 | 437.9 | |
| 0 | 7 | 0 | 5 | -21.75 | 302.34 | 38.95 | 234.27 | 0.7217 | -310.0 | -367.8 | |
| 0 | 6 | 0 | 4 | -22.45 | 300.65 | 37.27 | 232.33 | 0.7095 | 443.0 | 282.7 | |
| 2 | 29 | 1 | 20 | -22.68 | 300.21 | 36.82 | 231.73 | 0.7067 | 566.7 | 505.2 | |
| 8 | -16 | 5 | -16 | -22.48 | 299.57 | 36.19 | 231.53 | 0.6992 | 907.2 | 999999 | |
| 0 | 3 | 0 | 2 | -22.15 | 298.75 | 35.37 | 231.35 | 0.6888 | 628.0 | 590.6 | |
| 0 | 4 | 0 | 3 | -22.43 | 298.22 | 34.84 | 230.62 | 0.6855 | 500.0 | 476.0 | |
| 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. | |