SOHO MDI 2000-08-29 23:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 109 | 632 | 95 | 554 | 13.02 | 356.06 | -56.29 | 79.07 | 0.8263 | 161.4 | 29.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14 | 234 | 11 | 189 | 13.64 | 0.30 | -52.04 | 78.26 | 0.7849 | 1330.9 | 514.0 | |
| 13 | -1 | 10 | -1 | 13.42 | 359.71 | -52.64 | 78.56 | 0.7911 | 1006.6 | 999999 | |
| 11 | -1 | 9 | -1 | 13.71 | 358.59 | -53.75 | 78.22 | 0.8026 | 650.6 | 999999 | |
| 0 | 2 | 0 | 2 | 13.08 | 358.66 | -53.68 | 79.01 | 0.8017 | 421.0 | 345.5 | |
| 19 | 145 | 16 | 124 | 12.89 | 357.61 | -54.73 | 79.26 | 0.8123 | 901.7 | 165.3 | |
| 5 | -5 | 4 | -5 | 12.89 | 356.76 | -55.58 | 79.27 | 0.8207 | 304.5 | 999999 | |
| 1 | 8 | 1 | 7 | 14.00 | 355.86 | -56.49 | 77.93 | 0.8295 | 302.2 | 247.2 | |
| 5 | -5 | 5 | -5 | 12.60 | 355.92 | -56.43 | 79.62 | 0.8288 | 128.4 | 999999 | |
| 0 | 13 | 0 | 11 | 14.14 | 355.28 | -57.06 | 77.77 | 0.8349 | 263.0 | -23.3 | |
| 0 | 6 | 0 | 5 | 13.78 | 354.51 | -57.83 | 78.21 | 0.8420 | -204.0 | -211.8 | |
| 0 | 9 | 0 | 8 | 13.08 | 354.78 | -57.57 | 79.04 | 0.8395 | -446.0 | -430.2 | |
| 0 | 8 | 0 | 7 | 13.40 | 353.65 | -58.69 | 78.65 | 0.8498 | -564.0 | -674.5 | |
| 0 | 3 | 0 | 3 | 14.34 | 352.95 | -59.40 | 77.56 | 0.8560 | -832.0 | -670.9 | |
| 7 | 182 | 7 | 176 | 12.67 | 353.54 | -58.80 | 79.51 | 0.8508 | -739.5 | -470.0 | |
| 0 | 8 | 0 | 7 | 14.00 | 352.85 | -59.49 | 77.95 | 0.8569 | -761.0 | -641.2 | |
| 14 | -14 | 13 | -14 | 12.37 | 352.62 | -59.72 | 79.85 | 0.8590 | -1068.1 | 999999 | |
| 17 | -14 | 16 | -14 | 12.17 | 351.80 | -60.54 | 80.07 | 0.8661 | -677.7 | 999999 | |
| 0 | 5 | 0 | 5 | 13.26 | 351.19 | -61.15 | 78.79 | 0.8711 | -384.0 | -380.8 | |
| 3 | 9 | 3 | 10 | 12.52 | 349.16 | -63.18 | 79.59 | 0.8877 | -383.6 | -304.5 | |
| 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. | |