SOHO MDI 2000-07-09 22:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6 | 103 | 3 | 53 | 13.15 | 352.68 | -15.34 | 57.15 | 0.3079 | 898.8 | 287.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | 15.94 | 356.29 | -11.73 | 42.96 | 0.2882 | 731.0 | 603.6 | |
| 0 | 9 | 0 | 4 | 11.68 | 356.46 | -11.56 | 55.14 | 0.2402 | 868.0 | 646.0 | |
| 0 | 6 | 0 | 3 | 15.01 | 355.92 | -12.10 | 46.21 | 0.2817 | 977.0 | 717.8 | |
| 0 | 2 | 0 | 1 | 15.20 | 355.45 | -12.57 | 46.76 | 0.2896 | 694.0 | 621.5 | |
| 0 | 5 | 0 | 3 | 15.00 | 355.08 | -12.94 | 48.10 | 0.2919 | 1098.0 | 796.7 | |
| 0 | 5 | 0 | 2 | 14.19 | 355.09 | -12.93 | 50.28 | 0.2833 | 996.0 | 849.5 | |
| 0 | 8 | 0 | 4 | 14.83 | 354.67 | -13.35 | 49.40 | 0.2953 | 805.0 | 646.9 | |
| 0 | 4 | 0 | 2 | 12.89 | 354.37 | -13.65 | 55.50 | 0.2804 | 657.0 | 474.0 | |
| 0 | 4 | 0 | 2 | 12.79 | 353.12 | -14.90 | 58.00 | 0.2971 | 814.0 | 619.4 | |
| 6 | 25 | 3 | 13 | 12.06 | 352.57 | -15.45 | 61.01 | 0.2991 | 1305.3 | 808.0 | |
| 0 | 4 | 0 | 2 | 11.42 | 352.53 | -15.50 | 63.03 | 0.2951 | 1065.0 | 845.0 | |
| 0 | 13 | 0 | 7 | 12.32 | 351.17 | -16.86 | 62.23 | 0.3216 | -1250.0 | -885.6 | |
| 0 | 9 | 0 | 5 | 12.02 | 348.54 | -19.48 | 66.03 | 0.3585 | -1185.0 | -872.4 | |
| 0 | 5 | 0 | 3 | 16.10 | 344.04 | -23.98 | 60.95 | 0.4486 | -684.0 | -610.5 | |
| 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. | |