SOHO MDI 2000-11-06 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59 | 367 | 46 | 282 | -12.13 | 175.50 | -47.48 | 109.31 | 0.7657 | 421.3 | 87.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5 | 88 | 4 | 65 | -12.54 | 177.60 | -45.38 | 110.56 | 0.7444 | 1251.7 | 762.3 | |
| 7 | 61 | 5 | 46 | -13.73 | 177.09 | -45.89 | 111.88 | 0.7540 | 796.3 | 168.5 | |
| 6 | -1 | 5 | -1 | -12.36 | 177.30 | -45.68 | 110.21 | 0.7470 | 957.3 | 999999 | |
| 9 | 48 | 7 | 37 | -12.71 | 176.65 | -46.33 | 110.41 | 0.7552 | 961.8 | 658.5 | |
| 11 | -4 | 8 | -4 | -13.20 | 176.47 | -46.50 | 110.97 | 0.7587 | 824.2 | 999999 | |
| 0 | 11 | 0 | 8 | -13.86 | 175.95 | -47.02 | 111.61 | 0.7664 | -233.0 | -245.2 | |
| 7 | 18 | 5 | 14 | -12.80 | 175.59 | -47.39 | 110.14 | 0.7668 | 440.7 | 308.6 | |
| 0 | 4 | 0 | 3 | -11.96 | 175.49 | -47.48 | 109.06 | 0.7652 | 567.0 | 452.8 | |
| 0 | 3 | 0 | 3 | -12.30 | 175.06 | -47.92 | 109.34 | 0.7708 | 250.0 | 158.2 | |
| 0 | 4 | 0 | 3 | -10.28 | 175.16 | -47.82 | 106.81 | 0.7640 | -789.0 | -687.2 | |
| 0 | 6 | 0 | 5 | -10.45 | 174.77 | -48.21 | 106.91 | 0.7687 | -818.0 | -722.5 | |
| 7 | 81 | 6 | 64 | -10.84 | 173.43 | -49.55 | 106.99 | 0.7838 | -754.0 | -599.3 | |
| 0 | 12 | 0 | 9 | -10.32 | 173.55 | -49.43 | 106.38 | 0.7813 | -859.0 | -698.2 | |
| 2 | -12 | 2 | -12 | -10.58 | 173.00 | -49.97 | 106.55 | 0.7876 | -862.8 | 999999 | |
| 5 | 27 | 4 | 22 | -10.85 | 172.39 | -50.59 | 106.70 | 0.7945 | -654.3 | -448.6 | |
| 0 | 4 | 0 | 3 | -10.80 | 171.77 | -51.20 | 106.47 | 0.8006 | -452.0 | -367.5 | |
| 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. | |