SOHO MDI 2000-11-10 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56 | 410 | 28 | 210 | -12.43 | 176.77 | 3.86 | 193.49 | 0.2799 | 1494.8 | 484.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 8 | 0 | 4 | -12.92 | 179.16 | 6.25 | 200.89 | 0.2990 | -792.0 | -734.7 | |
| 12 | 322 | 6 | 166 | -13.28 | 177.70 | 4.80 | 195.98 | 0.2969 | 1274.8 | 710.4 | |
| 17 | -2 | 9 | -2 | -12.28 | 177.49 | 4.58 | 196.27 | 0.2798 | 1958.1 | 999999 | |
| 9 | -2 | 4 | -2 | -12.87 | 177.26 | 4.35 | 194.93 | 0.2884 | 1436.1 | 999999 | |
| 18 | -2 | 9 | -2 | -12.71 | 176.83 | 3.92 | 193.63 | 0.2840 | 1693.3 | 999999 | |
| 0 | 5 | 0 | 2 | -13.79 | 176.21 | 3.30 | 190.80 | 0.2995 | 569.0 | 570.0 | |
| 0 | 5 | 0 | 3 | -13.43 | 175.89 | 2.98 | 189.99 | 0.2925 | 774.0 | 678.4 | |
| 0 | 6 | 0 | 3 | -12.59 | 175.84 | 2.93 | 190.36 | 0.2785 | 919.0 | 790.7 | |
| 0 | 6 | 0 | 3 | -7.50 | 175.60 | 2.69 | 194.02 | 0.1928 | -334.0 | -356.2 | |
| 0 | 16 | 0 | 8 | -9.77 | 174.87 | 1.96 | 188.53 | 0.2287 | -734.0 | -587.2 | |
| 0 | 6 | 0 | 3 | -15.16 | 174.20 | 1.29 | 183.93 | 0.3178 | -694.0 | -573.2 | |
| 0 | 13 | 0 | 6 | -9.34 | 173.86 | 0.95 | 184.29 | 0.2194 | -501.0 | -506.3 | |
| 0 | 7 | 0 | 4 | -9.57 | 173.63 | 0.72 | 183.18 | 0.2231 | -870.0 | -740.0 | |
| 0 | 5 | 0 | 2 | -14.07 | 173.24 | 0.33 | 181.08 | 0.2989 | -894.0 | -707.9 | |
| 0 | 7 | 0 | 4 | -13.47 | 172.88 | -0.02 | 179.92 | 0.2888 | -862.0 | -697.8 | |
| 0 | 4 | 0 | 2 | -9.73 | 171.33 | -1.58 | 173.08 | 0.2271 | -655.0 | -568.0 | |
| 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. | |