SOHO MDI 2000-11-01 23:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 107 | 0 | 64 | -26.97 | 290.73 | 2.75 | 184.66 | 0.5225 | 650.4 | 585.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 2 | 0 | 1 | -28.60 | 295.89 | 7.91 | 192.59 | 0.5565 | 416.0 | 527.2 | |
| 0 | 9 | 0 | 6 | -28.73 | 294.93 | 6.95 | 191.05 | 0.5555 | 823.0 | 644.5 | |
| 0 | 4 | 0 | 2 | -28.91 | 294.14 | 6.16 | 189.77 | 0.5559 | 397.0 | 393.0 | |
| 0 | 3 | 0 | 2 | -25.51 | 292.97 | 4.99 | 189.01 | 0.5035 | 798.0 | 700.9 | |
| 0 | 18 | 0 | 10 | -26.89 | 292.51 | 4.53 | 187.77 | 0.5230 | 960.0 | 744.1 | |
| 0 | 4 | 0 | 2 | -25.42 | 292.45 | 4.47 | 188.12 | 0.5009 | 671.0 | 663.9 | |
| 0 | 5 | 0 | 3 | -25.11 | 292.14 | 4.16 | 187.65 | 0.4956 | 772.0 | 725.5 | |
| 0 | 5 | 0 | 3 | -27.47 | 291.19 | 3.20 | 185.40 | 0.5293 | 754.0 | 545.0 | |
| 0 | 5 | 0 | 3 | -26.89 | 291.13 | 3.14 | 185.42 | 0.5205 | 932.0 | 780.5 | |
| 0 | 3 | 0 | 2 | -27.51 | 290.19 | 2.21 | 183.72 | 0.5287 | 745.0 | 809.2 | |
| 0 | 5 | 0 | 3 | -26.97 | 290.09 | 2.11 | 183.63 | 0.5206 | 1110.0 | 1083.3 | |
| 0 | 3 | 0 | 2 | -27.38 | 289.49 | 1.51 | 182.56 | 0.5261 | 772.0 | 874.4 | |
| 0 | 5 | 0 | 3 | -26.88 | 289.40 | 1.42 | 182.45 | 0.5187 | 1069.0 | 923.0 | |
| 0 | 6 | 0 | 3 | -24.87 | 289.33 | 1.35 | 182.52 | 0.4883 | 955.0 | 745.5 | |
| 0 | 4 | 0 | 3 | -27.29 | 289.19 | 1.20 | 182.05 | 0.5246 | 872.0 | 797.6 | |
| 0 | 5 | 0 | 3 | -26.56 | 288.96 | 0.98 | 181.72 | 0.5137 | -274.0 | -148.8 | |
| 0 | 7 | 0 | 4 | -25.85 | 288.02 | 0.03 | 180.06 | 0.5027 | -803.0 | -689.1 | |
| 0 | 6 | 0 | 4 | -27.33 | 287.11 | -0.88 | 178.51 | 0.5251 | 722.0 | 616.6 | |
| 0 | 8 | 0 | 5 | -27.56 | 286.63 | -1.36 | 177.72 | 0.5287 | 667.0 | 540.6 | |
| 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. | |