SOHO MDI 2000-10-31 17:59:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8 | 143 | 5 | 85 | -27.67 | 292.61 | -11.84 | 161.02 | 0.5613 | 837.7 | 720.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 9 | 0 | 5 | -29.11 | 296.04 | -8.41 | 166.92 | 0.5671 | 889.0 | 691.9 | |
| 0 | 6 | 0 | 3 | -26.88 | 295.73 | -8.72 | 165.35 | 0.5368 | 585.0 | 686.1 | |
| 0 | 7 | 0 | 4 | -28.94 | 294.89 | -9.56 | 165.14 | 0.5687 | 790.0 | 784.7 | |
| 0 | 5 | 0 | 3 | -26.80 | 294.73 | -9.72 | 163.72 | 0.5396 | 702.0 | 794.7 | |
| 0 | 15 | 0 | 9 | -26.41 | 293.54 | -10.91 | 161.61 | 0.5394 | 802.0 | 736.1 | |
| 0 | 3 | 0 | 2 | -25.35 | 293.21 | -11.25 | 160.36 | 0.5263 | 835.0 | 750.1 | |
| 8 | 16 | 5 | 10 | -29.67 | 292.48 | -11.98 | 162.08 | 0.5883 | 891.2 | 640.9 | |
| 0 | 4 | 0 | 2 | -27.01 | 292.69 | -11.76 | 160.70 | 0.5517 | 688.0 | 646.4 | |
| 0 | 4 | 0 | 2 | -26.52 | 292.70 | -11.75 | 160.37 | 0.5449 | 1005.0 | 916.2 | |
| 0 | 5 | 0 | 3 | -29.08 | 291.91 | -12.54 | 160.93 | 0.5830 | 797.0 | 523.0 | |
| 0 | 12 | 0 | 7 | -26.53 | 292.04 | -12.42 | 159.38 | 0.5484 | 864.0 | 927.6 | |
| 0 | 16 | 0 | 9 | -26.76 | 291.79 | -12.66 | 159.17 | 0.5527 | 1027.0 | 840.2 | |
| 0 | 5 | 0 | 3 | -29.55 | 291.31 | -13.14 | 160.41 | 0.5921 | 508.0 | 494.0 | |
| 0 | 13 | 0 | 8 | -27.71 | 291.50 | -12.95 | 159.43 | 0.5669 | 781.0 | 662.7 | |
| 0 | 10 | 0 | 6 | -27.26 | 291.38 | -13.08 | 158.93 | 0.5616 | 1075.0 | 880.1 | |
| 0 | 3 | 0 | 2 | -29.05 | 291.10 | -13.35 | 159.79 | 0.5865 | 617.0 | 518.2 | |
| 0 | 3 | 0 | 2 | -27.86 | 291.03 | -13.42 | 158.87 | 0.5712 | 762.0 | 694.2 | |
| 0 | 4 | 0 | 3 | -28.41 | 290.87 | -13.58 | 159.03 | 0.5793 | 518.0 | 514.7 | |
| 0 | 3 | 0 | 2 | -25.37 | 289.79 | -14.66 | 155.12 | 0.5457 | 498.0 | 424.7 | |
| 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. | |