SOHO MDI 2000-01-24 19:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 203 | 22 | 110 | -16.88 | 76.57 | 21.83 | 239.80 | 0.4135 | -385.8 | -150.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7 | 80 | 4 | 44 | -16.27 | 79.09 | 24.35 | 243.55 | 0.4439 | -1092.9 | -906.1 | |
| 7 | -1 | 4 | -1 | -16.25 | 78.60 | 23.86 | 243.20 | 0.4370 | -1116.0 | 999999 | |
| 4 | -1 | 2 | -1 | -16.03 | 78.27 | 23.53 | 243.39 | 0.4310 | -1431.4 | 999999 | |
| 0 | 4 | 0 | 2 | -16.24 | 77.91 | 23.17 | 242.63 | 0.4272 | -518.0 | -345.7 | |
| 0 | 3 | 0 | 1 | -17.03 | 77.53 | 22.79 | 240.57 | 0.4271 | -754.0 | -640.3 | |
| 0 | 5 | 0 | 3 | -15.85 | 76.65 | 21.91 | 242.33 | 0.4071 | -602.0 | -531.1 | |
| 0 | 8 | 0 | 4 | -15.49 | 75.84 | 21.10 | 242.38 | 0.3933 | 756.0 | 570.9 | |
| 0 | 5 | 0 | 3 | -17.79 | 76.02 | 21.28 | 237.41 | 0.4120 | 658.0 | 520.1 | |
| 2 | 10 | 1 | 6 | -15.62 | 75.56 | 20.82 | 241.80 | 0.3901 | 839.1 | 626.8 | |
| 12 | 46 | 6 | 25 | -18.32 | 75.66 | 20.92 | 235.88 | 0.4112 | 17.1 | 71.4 | |
| 2 | -10 | 1 | -10 | -17.88 | 75.60 | 20.86 | 236.74 | 0.4071 | 1072.2 | 999999 | |
| 3 | -10 | 2 | -10 | -18.63 | 75.57 | 20.83 | 235.11 | 0.4126 | -945.4 | 999999 | |
| 0 | 4 | 0 | 2 | -15.75 | 75.10 | 20.36 | 241.02 | 0.3845 | 315.0 | 365.3 | |
| 0 | 12 | 0 | 6 | -16.81 | 73.52 | 18.78 | 236.64 | 0.3706 | 1123.0 | 877.5 | |
| 0 | 13 | 0 | 7 | -17.36 | 73.49 | 18.75 | 235.33 | 0.3747 | 1039.0 | 844.0 | |
| 5 | 13 | 2 | 7 | -17.79 | 73.41 | 18.67 | 234.23 | 0.3773 | 1033.2 | 710.1 | |
| 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. | |