SOHO MDI 2000-07-19 11:11:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55 | 336 | 41 | 254 | 18.81 | 290.18 | 48.37 | 290.82 | 0.7585 | 108.9 | 174.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12 | 228 | 9 | 178 | 18.39 | 292.19 | 50.38 | 289.82 | 0.7793 | 605.1 | 431.6 | |
| 13 | -1 | 10 | -1 | 19.08 | 291.75 | 49.94 | 290.78 | 0.7760 | 732.0 | 999999 | |
| 6 | -1 | 5 | -1 | 18.61 | 291.24 | 49.43 | 290.29 | 0.7698 | 1216.3 | 999999 | |
| 0 | 8 | 0 | 6 | 18.89 | 290.13 | 48.33 | 290.88 | 0.7587 | 665.0 | 559.0 | |
| 7 | 13 | 5 | 10 | 18.72 | 288.03 | 46.22 | 291.16 | 0.7356 | -466.3 | -339.3 | |
| 0 | 4 | 0 | 3 | 18.64 | 287.46 | 45.65 | 291.19 | 0.7290 | -565.0 | -403.9 | |
| 0 | 6 | 0 | 4 | 18.21 | 286.36 | 44.56 | 290.89 | 0.7157 | -641.0 | -555.3 | |
| 0 | 6 | 0 | 4 | 20.64 | 287.11 | 45.30 | 293.98 | 0.7303 | -376.0 | -264.1 | |
| 0 | 4 | 0 | 3 | 18.94 | 286.37 | 44.57 | 291.90 | 0.7177 | -223.0 | -205.9 | |
| 0 | 4 | 0 | 3 | 17.62 | 285.83 | 44.02 | 290.22 | 0.7082 | 395.0 | 305.7 | |
| 11 | 49 | 8 | 34 | 19.02 | 285.70 | 43.89 | 292.20 | 0.7102 | -834.1 | -652.9 | |
| 6 | -11 | 4 | -11 | 19.01 | 285.17 | 43.37 | 292.34 | 0.7042 | -1120.4 | 999999 | |
| 0 | 2 | 0 | 1 | 19.89 | 284.89 | 43.08 | 293.65 | 0.7035 | -416.0 | -472.1 | |
| 0 | 4 | 0 | 3 | 19.25 | 284.56 | 42.75 | 292.86 | 0.6978 | -789.0 | -742.2 | |
| 0 | 5 | 0 | 3 | 19.62 | 284.68 | 42.87 | 293.33 | 0.7003 | -681.0 | -657.0 | |
| 0 | 3 | 0 | 2 | 19.88 | 284.37 | 42.56 | 293.80 | 0.6975 | -772.0 | -651.1 | |
| 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. | |