SOHO MDI 2000-08-29 04:47:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50 | 303 | 62 | 367 | 13.00 | 356.12 | -66.80 | 78.89 | 0.9125 | 93.9 | 92.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15 | 153 | 16 | 164 | 13.67 | 0.07 | -62.85 | 78.29 | 0.8849 | 951.3 | 435.0 | |
| -1 | -1 | -1 | -1 | 13.46 | 359.62 | -63.29 | 78.52 | 0.8884 | 999999 | 999999 | |
| 0 | 5 | 0 | 5 | 12.38 | 359.30 | -63.61 | 79.73 | 0.8911 | 239.0 | 216.2 | |
| 5 | -1 | 5 | -1 | 13.60 | 358.63 | -64.28 | 78.35 | 0.8960 | 275.8 | 999999 | |
| 0 | 6 | 0 | 7 | 14.02 | 358.42 | -64.50 | 77.87 | 0.8976 | -27.0 | -73.2 | |
| 0 | 2 | 0 | 2 | 13.17 | 358.47 | -64.45 | 78.81 | 0.8973 | -191.0 | -131.0 | |
| 9 | 32 | 11 | 38 | 12.65 | 356.68 | -66.24 | 79.33 | 0.9105 | 456.8 | 249.9 | |
| 0 | 6 | 0 | 7 | 14.34 | 354.86 | -68.06 | 77.42 | 0.9224 | 79.0 | 36.4 | |
| 0 | 2 | 0 | 2 | 13.36 | 353.68 | -69.23 | 78.43 | 0.9302 | -422.0 | -386.3 | |
| 8 | 81 | 11 | 115 | 12.62 | 353.21 | -69.71 | 79.21 | 0.9333 | -662.5 | -423.8 | |
| 9 | -10 | 12 | -10 | 12.03 | 352.00 | -70.92 | 79.76 | 0.9408 | -524.4 | 999999 | |
| 3 | -10 | 5 | -10 | 12.29 | 351.83 | -71.09 | 79.47 | 0.9416 | -406.3 | 999999 | |
| 1 | 13 | 2 | 22 | 12.48 | 349.27 | -73.65 | 79.12 | 0.9554 | -11.7 | 74.3 | |
| 0 | 3 | 0 | 5 | 12.04 | 349.01 | -73.91 | 79.56 | 0.9568 | 56.0 | 67.1 | |
| 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. | |