SOHO MDI 2000-09-07 01:24:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48 | 214 | 30 | 127 | 10.30 | 340.61 | 34.74 | 277.79 | 0.5677 | 144.7 | -39.2 | |
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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 | 7.12 | 346.74 | 40.87 | 272.48 | 0.6523 | -542.0 | -548.3 | |
| 8 | 18 | 5 | 11 | 8.76 | 344.00 | 38.13 | 274.95 | 0.6148 | 845.1 | 512.2 | |
| 0 | 9 | 0 | 6 | 9.00 | 343.42 | 37.55 | 275.34 | 0.6069 | 918.0 | 774.9 | |
| 10 | 63 | 6 | 39 | 9.54 | 343.04 | 37.17 | 276.24 | 0.6016 | 1089.2 | 708.4 | |
| 10 | -4 | 6 | -4 | 9.57 | 342.69 | 36.83 | 276.29 | 0.5969 | 1418.5 | 999999 | |
| 0 | 5 | 0 | 3 | 8.91 | 341.97 | 36.10 | 275.18 | 0.5867 | 838.0 | 637.1 | |
| 0 | 5 | 0 | 3 | 9.79 | 340.12 | 34.26 | 276.77 | 0.5608 | -501.0 | -448.8 | |
| 0 | 7 | 0 | 4 | 11.51 | 339.28 | 33.42 | 279.94 | 0.5500 | -534.0 | -502.2 | |
| 0 | 4 | 0 | 2 | 10.78 | 339.00 | 33.13 | 278.64 | 0.5452 | -494.0 | -520.9 | |
| 4 | 39 | 3 | 23 | 11.54 | 338.76 | 32.89 | 280.07 | 0.5426 | -1106.3 | -814.2 | |
| 5 | 16 | 3 | 9 | 10.70 | 338.41 | 32.55 | 278.55 | 0.5367 | -1044.8 | -724.2 | |
| 5 | -10 | 3 | -10 | 11.53 | 338.28 | 32.42 | 280.13 | 0.5357 | -1026.3 | 999999 | |
| 0 | 8 | 0 | 4 | 10.91 | 337.54 | 31.68 | 279.06 | 0.5242 | 36.0 | 128.9 | |
| 6 | 37 | 4 | 21 | 11.52 | 337.34 | 31.47 | 280.25 | 0.5219 | -1285.1 | -694.0 | |
| 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. | |