SOHO MDI 2000-07-08 15:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 36 | 0 | 37 | -12.34 | 324.30 | -60.50 | 106.09 | 0.8862 | -297.0 | -293.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 14 | 0 | 14 | -12.86 | 325.70 | -59.10 | 106.95 | 0.8765 | -542.0 | -521.6 | |
| 0 | 8 | 0 | 8 | -12.27 | 325.12 | -59.68 | 106.17 | 0.8802 | -491.0 | -311.2 | |
| 0 | 4 | 0 | 4 | -12.40 | 324.41 | -60.38 | 106.16 | 0.8859 | -121.0 | -20.2 | |
| 0 | 6 | 0 | 6 | -11.74 | 324.41 | -60.38 | 105.43 | 0.8849 | -456.0 | -271.8 | |
| 0 | 4 | 0 | 5 | -11.67 | 318.83 | -65.96 | 104.30 | 0.9247 | 125.0 | 130.0 | |
| 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. | |