SOHO MDI 2000-10-04 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 101 | 655 | 86 | 586 | -12.31 | 351.32 | 53.36 | 250.28 | 0.8313 | 297.5 | 48.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13 | 199 | 14 | 213 | -11.09 | 358.58 | 60.62 | 253.98 | 0.8915 | -510.2 | -235.9 | |
| 9 | -1 | 10 | -1 | -11.22 | 357.90 | 59.94 | 253.66 | 0.8866 | -904.1 | 999999 | |
| 0 | 83 | 0 | 73 | -13.12 | 350.65 | 52.69 | 249.33 | 0.8300 | -301.0 | -462.4 | |
| 7 | 16 | 6 | 14 | -11.82 | 349.82 | 51.86 | 250.55 | 0.8186 | -698.2 | -571.8 | |
| 8 | 137 | 6 | 113 | -12.75 | 347.91 | 49.95 | 248.77 | 0.8032 | -175.4 | 198.5 | |
| 7 | -5 | 6 | -5 | -13.37 | 347.59 | 49.63 | 247.90 | 0.8022 | 719.2 | 999999 | |
| 0 | 8 | 0 | 7 | -11.52 | 346.93 | 48.96 | 249.86 | 0.7895 | -60.0 | -109.4 | |
| 3 | -5 | 2 | -5 | -13.67 | 347.18 | 49.22 | 247.39 | 0.7992 | 703.3 | 999999 | |
| 0 | 5 | 0 | 4 | -11.69 | 346.48 | 48.52 | 249.49 | 0.7856 | 525.0 | 450.4 | |
| 4 | -5 | 3 | -5 | -13.50 | 346.70 | 48.74 | 247.40 | 0.7941 | 830.9 | 999999 | |
| 0 | 10 | 0 | 8 | -13.85 | 346.50 | 48.53 | 246.89 | 0.7933 | 534.0 | 352.0 | |
| 5 | 133 | 4 | 104 | -12.61 | 345.87 | 47.90 | 248.13 | 0.7826 | 834.7 | 689.9 | |
| 13 | -12 | 10 | -12 | -12.30 | 345.61 | 47.65 | 248.39 | 0.7789 | 1075.2 | 999999 | |
| 14 | -12 | 11 | -12 | -12.92 | 345.65 | 47.68 | 247.66 | 0.7815 | 963.5 | 999999 | |
| 5 | 60 | 4 | 47 | -13.61 | 345.59 | 47.63 | 246.80 | 0.7835 | 868.6 | 462.3 | |
| 9 | -12 | 7 | -12 | -11.97 | 345.12 | 47.16 | 248.59 | 0.7728 | 1197.8 | 999999 | |
| 4 | -15 | 3 | -15 | -14.00 | 345.40 | 47.43 | 246.25 | 0.7831 | 785.3 | 999999 | |
| 0 | 4 | 0 | 3 | -14.16 | 344.85 | 46.89 | 245.82 | 0.7782 | 232.0 | 134.2 | |
| 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. | |