SOHO MDI 2000-11-02 17:51:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3 | 103 | 2 | 61 | -27.07 | 290.82 | 12.65 | 200.61 | 0.5542 | 790.5 | 712.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 3 | -30.46 | 295.60 | 17.43 | 204.57 | 0.6231 | 561.0 | 427.7 | |
| 0 | 5 | 0 | 3 | -26.53 | 293.59 | 15.42 | 205.13 | 0.5626 | 859.0 | 789.9 | |
| 0 | 5 | 0 | 3 | -27.10 | 292.87 | 14.70 | 203.64 | 0.5656 | 798.0 | 727.4 | |
| 0 | 4 | 0 | 3 | -27.63 | 292.36 | 14.19 | 202.50 | 0.5696 | 518.0 | 501.2 | |
| 0 | 4 | 0 | 2 | -25.74 | 291.85 | 13.68 | 203.25 | 0.5419 | 812.0 | 773.5 | |
| 0 | 4 | 0 | 2 | -26.36 | 291.62 | 13.45 | 202.41 | 0.5488 | 827.0 | 748.3 | |
| 0 | 7 | 0 | 4 | -27.34 | 291.65 | 13.48 | 201.71 | 0.5620 | 666.0 | 578.4 | |
| 0 | 12 | 0 | 7 | -26.89 | 291.19 | 13.02 | 201.38 | 0.5535 | 1167.0 | 944.1 | |
| 0 | 8 | 0 | 5 | -27.15 | 290.83 | 12.65 | 200.64 | 0.5551 | 891.0 | 878.4 | |
| 0 | 4 | 0 | 3 | -28.50 | 290.14 | 11.96 | 198.72 | 0.5699 | 661.0 | 588.0 | |
| 0 | 6 | 0 | 4 | -27.00 | 289.84 | 11.66 | 199.27 | 0.5482 | 1076.0 | 957.7 | |
| 0 | 9 | 0 | 5 | -27.36 | 289.83 | 11.66 | 199.02 | 0.5530 | 852.0 | 714.9 | |
| 3 | 9 | 2 | 5 | -25.74 | 289.45 | 11.27 | 199.53 | 0.5290 | 848.9 | 660.9 | |
| 0 | 10 | 0 | 6 | -26.81 | 289.11 | 10.94 | 198.28 | 0.5421 | 1222.0 | 1039.6 | |
| 0 | 6 | 0 | 3 | -27.12 | 289.01 | 10.84 | 197.93 | 0.5460 | 886.0 | 776.1 | |
| 0 | 5 | 0 | 3 | -25.76 | 287.58 | 9.41 | 196.49 | 0.5207 | -522.0 | -427.5 | |
| 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. | |