SOHO MDI 2000-09-07 11:32:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49 | 250 | 31 | 162 | 10.28 | 340.62 | 40.33 | 277.49 | 0.6443 | -120.3 | -190.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 10 | 0 | 7 | 6.97 | 346.96 | 46.67 | 272.72 | 0.7252 | -330.0 | -309.3 | |
| 6 | 21 | 4 | 14 | 8.65 | 345.43 | 45.14 | 274.98 | 0.7058 | 534.4 | 488.0 | |
| 15 | 44 | 10 | 29 | 9.36 | 343.16 | 42.87 | 275.95 | 0.6772 | 1086.7 | 591.4 | |
| 0 | 4 | 0 | 3 | 8.62 | 342.56 | 42.27 | 274.83 | 0.6698 | 800.0 | 621.8 | |
| 0 | 6 | 0 | 4 | 10.24 | 342.00 | 41.71 | 277.28 | 0.6624 | 490.0 | 380.3 | |
| 0 | 8 | 0 | 5 | 3.89 | 341.25 | 40.96 | 267.55 | 0.6570 | -812.0 | -576.9 | |
| 0 | 4 | 0 | 3 | 9.04 | 341.29 | 41.00 | 275.44 | 0.6531 | 623.0 | 641.0 | |
| 0 | 3 | 0 | 2 | 9.62 | 340.90 | 40.61 | 276.34 | 0.6480 | 489.0 | 621.9 | |
| 0 | 6 | 0 | 4 | 9.69 | 339.66 | 39.37 | 276.44 | 0.6315 | 479.0 | 393.2 | |
| 0 | 9 | 0 | 6 | 10.90 | 339.74 | 39.45 | 278.37 | 0.6329 | -115.0 | -29.7 | |
| 0 | 5 | 0 | 3 | 10.91 | 339.12 | 38.83 | 278.42 | 0.6247 | -407.0 | -208.8 | |
| 3 | 96 | 2 | 61 | 11.99 | 338.99 | 38.70 | 280.16 | 0.6236 | -775.6 | -682.8 | |
| 9 | -12 | 5 | -12 | 11.45 | 338.74 | 38.45 | 279.32 | 0.6199 | -994.4 | 999999 | |
| 4 | -12 | 2 | -12 | 11.70 | 338.17 | 37.88 | 279.76 | 0.6124 | -977.4 | 999999 | |
| 3 | 34 | 2 | 21 | 11.54 | 337.64 | 37.35 | 279.55 | 0.6050 | -902.1 | -732.5 | |
| 9 | -15 | 6 | -15 | 11.69 | 337.21 | 36.92 | 279.84 | 0.5993 | -1152.1 | 999999 | |
| 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. | |