SOHO MDI 2000-07-09 14:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17 | 93 | 9 | 51 | 13.28 | 350.64 | -21.80 | 64.29 | 0.4015 | 309.7 | 287.5 | |
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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 | 15.84 | 356.21 | -16.22 | 52.00 | 0.3426 | 809.0 | 706.1 | |
| 0 | 8 | 0 | 4 | 11.38 | 356.27 | -16.16 | 63.97 | 0.3050 | 1081.0 | 932.8 | |
| 0 | 7 | 0 | 4 | 15.10 | 355.59 | -16.85 | 54.78 | 0.3440 | 1045.0 | 955.4 | |
| 0 | 4 | 0 | 2 | 15.21 | 355.15 | -17.29 | 55.16 | 0.3509 | 1039.0 | 860.0 | |
| 0 | 4 | 0 | 2 | 14.88 | 354.92 | -17.52 | 56.29 | 0.3512 | 914.0 | 871.9 | |
| 6 | 24 | 3 | 13 | 12.01 | 352.27 | -20.17 | 66.63 | 0.3689 | 1153.2 | 690.6 | |
| 6 | -6 | 3 | -6 | 11.73 | 352.21 | -20.23 | 67.41 | 0.3683 | 943.0 | 999999 | |
| 0 | 5 | 0 | 3 | 15.18 | 351.90 | -20.54 | 59.39 | 0.3951 | 680.0 | 612.8 | |
| 0 | 3 | 0 | 2 | 12.63 | 351.09 | -21.35 | 66.18 | 0.3899 | -640.0 | -607.2 | |
| 0 | 2 | 0 | 1 | 12.25 | 350.25 | -22.19 | 67.80 | 0.4002 | 536.0 | 525.2 | |
| 5 | 17 | 3 | 9 | 12.08 | 348.33 | -24.11 | 69.61 | 0.4279 | -1273.9 | -842.2 | |
| 0 | 8 | 0 | 4 | 16.81 | 347.18 | -25.26 | 60.61 | 0.4707 | -347.0 | -236.9 | |
| 0 | 3 | 0 | 2 | 18.27 | 342.96 | -29.48 | 61.18 | 0.5355 | -643.0 | -541.9 | |
| 0 | 4 | 0 | 3 | 9.95 | 335.20 | -37.24 | 78.66 | 0.6102 | 536.0 | 573.2 | |
| 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. | |