SOHO MDI 2000-09-05 09:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29 | 155 | 15 | 79 | 10.46 | 340.25 | 12.47 | 287.02 | 0.2250 | 28.0 | -10.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | 5.44 | 348.17 | 20.39 | 266.07 | 0.3491 | -601.0 | -484.6 | |
| 0 | 6 | 0 | 3 | 6.52 | 345.74 | 17.96 | 268.74 | 0.3078 | -555.0 | -379.3 | |
| 0 | 5 | 0 | 2 | 8.77 | 342.98 | 15.20 | 276.80 | 0.2622 | 1119.0 | 820.2 | |
| 7 | 16 | 3 | 8 | 9.52 | 342.85 | 15.07 | 279.71 | 0.2613 | 1071.4 | 796.0 | |
| 3 | 10 | 2 | 5 | 11.09 | 341.65 | 13.87 | 286.70 | 0.2467 | 1025.8 | 714.9 | |
| 0 | 5 | 0 | 3 | 11.57 | 341.51 | 13.73 | 288.72 | 0.2466 | 752.0 | 550.4 | |
| 6 | 18 | 3 | 9 | 9.65 | 341.22 | 13.43 | 281.18 | 0.2345 | 1274.4 | 958.6 | |
| 0 | 6 | 0 | 3 | 10.36 | 341.21 | 13.42 | 284.15 | 0.2366 | 790.0 | 630.9 | |
| 2 | 54 | 1 | 27 | 10.88 | 339.31 | 11.53 | 288.54 | 0.2079 | -1038.3 | -953.2 | |
| 0 | 10 | 0 | 5 | 11.40 | 339.16 | 11.38 | 291.11 | 0.2083 | -866.0 | -594.2 | |
| 3 | -9 | 2 | -9 | 10.57 | 339.09 | 11.31 | 287.37 | 0.2029 | -1353.4 | 999999 | |
| 8 | -9 | 4 | -9 | 10.97 | 338.82 | 11.04 | 289.66 | 0.2005 | -1395.4 | 999999 | |
| 0 | 5 | 0 | 3 | 11.52 | 337.09 | 9.31 | 295.62 | 0.1767 | 643.0 | 657.5 | |
| 0 | 6 | 0 | 3 | 9.54 | 336.19 | 8.41 | 285.93 | 0.1507 | 709.0 | 470.2 | |
| 0 | 6 | 0 | 3 | 14.99 | 334.85 | 7.07 | 318.75 | 0.1811 | 746.0 | 646.4 | |
| 0 | 3 | 0 | 2 | 15.43 | 334.78 | 7.00 | 320.60 | 0.1860 | 830.0 | 710.9 | |
| 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. | |