SOHO MDI 2000-07-13 09:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41 | 209 | 22 | 110 | -10.31 | 306.83 | -15.29 | 133.98 | 0.3614 | -393.0 | -347.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 9 | 0 | 4 | -10.32 | 311.07 | -11.05 | 142.99 | 0.3147 | -978.0 | -872.2 | |
| 0 | 6 | 0 | 3 | -9.51 | 310.65 | -11.47 | 140.31 | 0.3086 | -1285.0 | -931.0 | |
| 0 | 4 | 0 | 2 | -9.64 | 310.19 | -11.93 | 139.48 | 0.3151 | -1066.0 | -800.1 | |
| 4 | 9 | 2 | 5 | -10.05 | 309.69 | -12.44 | 139.16 | 0.3258 | -825.6 | -660.1 | |
| 0 | 3 | 0 | 1 | -10.27 | 309.10 | -13.03 | 138.29 | 0.3348 | -463.0 | -487.2 | |
| 0 | 4 | 0 | 2 | -9.21 | 308.98 | -13.15 | 135.80 | 0.3235 | 640.0 | 457.8 | |
| 0 | 5 | 0 | 3 | -10.60 | 308.71 | -13.41 | 138.13 | 0.3431 | -342.0 | -279.8 | |
| 5 | 15 | 3 | 8 | -10.25 | 307.69 | -14.43 | 135.34 | 0.3504 | 1298.1 | 791.8 | |
| 11 | 71 | 6 | 38 | -9.87 | 306.42 | -15.71 | 132.13 | 0.3612 | 923.1 | 62.0 | |
| 8 | 64 | 4 | 34 | -10.81 | 306.33 | -15.80 | 133.88 | 0.3726 | -1544.0 | -973.4 | |
| 13 | -10 | 7 | -10 | -10.82 | 305.99 | -16.13 | 133.30 | 0.3766 | -1443.6 | 999999 | |
| -11 | -10 | -11 | -10 | -10.82 | 305.78 | -16.34 | 132.94 | 0.3791 | 999999 | 999999 | |
| 0 | 4 | 0 | 2 | -10.88 | 305.23 | -16.89 | 132.10 | 0.3863 | -902.0 | -768.6 | |
| 0 | 9 | 0 | 5 | -11.06 | 304.59 | -17.54 | 131.39 | 0.3959 | -653.0 | -623.8 | |
| 0 | 6 | 0 | 3 | -10.81 | 303.03 | -19.10 | 128.52 | 0.4125 | 776.0 | 816.1 | |
| 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. | |