SOHO MDI 2000-09-06 05:56:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45 | 228 | 24 | 123 | 10.40 | 340.17 | 23.59 | 279.72 | 0.4013 | -278.0 | 10.7 | |
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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 | 6.82 | 346.41 | 29.83 | 271.05 | 0.4961 | -619.0 | -452.7 | |
| 0 | 4 | 0 | 2 | 7.24 | 346.03 | 29.45 | 271.86 | 0.4900 | -730.0 | -626.2 | |
| 0 | 4 | 0 | 2 | 8.97 | 343.96 | 27.38 | 275.52 | 0.4583 | 435.0 | 412.8 | |
| 0 | 4 | 0 | 2 | 3.92 | 343.05 | 26.47 | 264.22 | 0.4488 | -526.0 | -493.1 | |
| 4 | 79 | 2 | 43 | 9.53 | 342.40 | 25.82 | 276.92 | 0.4346 | 1275.9 | 991.3 | |
| 9 | -5 | 5 | -5 | 10.18 | 341.97 | 25.39 | 278.50 | 0.4285 | 1224.9 | 999999 | |
| 4 | -5 | 2 | -5 | 9.17 | 341.71 | 25.13 | 276.16 | 0.4235 | 1161.0 | 999999 | |
| 4 | -5 | 2 | -5 | 9.81 | 341.59 | 25.01 | 277.69 | 0.4221 | 1183.3 | 999999 | |
| 0 | 10 | 0 | 6 | 9.69 | 340.92 | 24.34 | 277.50 | 0.4115 | 960.0 | 770.6 | |
| 0 | 4 | 0 | 2 | 9.64 | 340.35 | 23.77 | 277.47 | 0.4025 | 270.0 | 393.5 | |
| 0 | 5 | 0 | 3 | 11.30 | 340.18 | 23.60 | 281.64 | 0.4026 | -588.0 | -412.6 | |
| 0 | 4 | 0 | 2 | 11.42 | 339.41 | 22.83 | 282.20 | 0.3907 | -565.0 | -529.7 | |
| 24 | 103 | 13 | 55 | 11.30 | 338.49 | 21.91 | 282.26 | 0.3761 | -1579.9 | -803.7 | |
| -13 | -13 | -13 | -13 | 11.03 | 338.34 | 21.76 | 281.60 | 0.3730 | 999999 | 999999 | |
| 0 | 3 | 0 | 2 | 13.22 | 335.05 | 18.47 | 289.67 | 0.3290 | 707.0 | 586.6 | |
| 0 | 4 | 0 | 2 | 14.61 | 334.95 | 18.37 | 293.75 | 0.3347 | 382.0 | 462.2 | |
| 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. | |