SOHO MDI 2000-11-01 20:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 121 | 0 | 70 | -26.67 | 291.71 | 1.97 | 183.42 | 0.5174 | 696.5 | 636.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 8 | 0 | 5 | -25.74 | 296.54 | 6.80 | 192.07 | 0.5120 | 721.0 | 578.2 | |
| 0 | 5 | 0 | 3 | -28.70 | 295.00 | 5.26 | 188.43 | 0.5512 | 720.0 | 646.7 | |
| 0 | 3 | 0 | 2 | -28.29 | 294.41 | 4.67 | 187.61 | 0.5439 | 803.0 | 671.9 | |
| 0 | 9 | 0 | 5 | -27.42 | 292.98 | 3.24 | 185.47 | 0.5287 | 709.0 | 624.3 | |
| 0 | 4 | 0 | 2 | -25.53 | 292.88 | 3.15 | 185.70 | 0.5005 | 849.0 | 708.4 | |
| 0 | 23 | 0 | 13 | -26.69 | 292.79 | 3.05 | 185.29 | 0.5177 | 861.0 | 773.6 | |
| 0 | 3 | 0 | 2 | -25.35 | 292.54 | 2.80 | 185.12 | 0.4973 | 777.0 | 751.5 | |
| 0 | 8 | 0 | 5 | -25.00 | 292.19 | 2.45 | 184.55 | 0.4914 | 832.0 | 757.2 | |
| 0 | 6 | 0 | 4 | -26.60 | 292.09 | 2.36 | 184.11 | 0.5155 | 1089.0 | 878.1 | |
| 0 | 6 | 0 | 3 | -26.87 | 291.93 | 2.19 | 183.78 | 0.5193 | 906.0 | 684.2 | |
| 0 | 5 | 0 | 3 | -27.46 | 291.16 | 1.42 | 182.40 | 0.5275 | 777.0 | 676.4 | |
| 0 | 8 | 0 | 4 | -26.91 | 290.11 | 0.38 | 180.65 | 0.5189 | 1129.0 | 1012.5 | |
| 0 | 4 | 0 | 2 | -26.91 | 289.42 | -0.31 | 179.46 | 0.5189 | 1092.0 | 854.8 | |
| 0 | 3 | 0 | 2 | -27.36 | 289.29 | -0.45 | 179.24 | 0.5257 | 768.0 | 792.0 | |
| 0 | 7 | 0 | 4 | -24.86 | 289.22 | -0.52 | 179.03 | 0.4879 | 969.0 | 790.7 | |
| 0 | 5 | 0 | 3 | -26.51 | 288.86 | -0.87 | 178.47 | 0.5130 | -282.0 | -205.4 | |
| 0 | 6 | 0 | 3 | -25.79 | 288.01 | -1.72 | 176.90 | 0.5028 | -857.0 | -592.9 | |
| 0 | 5 | 0 | 3 | -29.52 | 287.42 | -2.31 | 176.38 | 0.5585 | 439.0 | 371.0 | |
| 0 | 3 | 0 | 2 | -27.28 | 287.39 | -2.35 | 176.00 | 0.5256 | 932.0 | 821.4 | |
| 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. | |