SOHO MDI 2000-10-31 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59 | 470 | 37 | 305 | 9.80 | 267.61 | -39.70 | 79.89 | 0.6413 | 882.5 | 403.6 | |
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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 | 10.38 | 272.25 | -35.05 | 78.13 | 0.5795 | 415.0 | 468.7 | |
| 0 | 9 | 0 | 6 | 9.64 | 272.06 | -35.25 | 79.45 | 0.5810 | 844.0 | 814.3 | |
| 0 | 4 | 0 | 3 | 10.01 | 271.68 | -35.63 | 78.88 | 0.5869 | 573.0 | 602.2 | |
| 0 | 6 | 0 | 4 | 9.15 | 271.59 | -35.72 | 80.36 | 0.5869 | 586.0 | 626.5 | |
| 4 | 12 | 3 | 8 | 9.48 | 270.19 | -37.12 | 80.03 | 0.6067 | 820.0 | 681.6 | |
| 0 | 4 | 0 | 3 | 6.38 | 270.12 | -37.18 | 85.16 | 0.6051 | 451.0 | 354.5 | |
| 19 | 259 | 12 | 165 | 9.84 | 268.75 | -38.56 | 79.66 | 0.6266 | 1685.3 | 556.2 | |
| 8 | -7 | 5 | -7 | 9.55 | 268.34 | -38.97 | 80.18 | 0.6317 | 1070.0 | 999999 | |
| 8 | -7 | 5 | -7 | 9.76 | 267.95 | -39.35 | 79.89 | 0.6371 | 1066.8 | 999999 | |
| 0 | 6 | 0 | 4 | 8.78 | 267.73 | -39.58 | 81.46 | 0.6390 | -261.0 | -215.7 | |
| 4 | -7 | 2 | -7 | 9.59 | 267.52 | -39.79 | 80.23 | 0.6426 | 787.9 | 999999 | |
| 0 | 3 | 0 | 2 | 6.83 | 267.30 | -40.01 | 84.55 | 0.6436 | -631.0 | -601.0 | |
| 0 | 7 | 0 | 4 | 11.18 | 265.98 | -41.33 | 78.01 | 0.6647 | -679.0 | -526.5 | |
| 10 | 67 | 6 | 44 | 9.17 | 266.19 | -41.12 | 81.01 | 0.6596 | -604.9 | 303.0 | |
| 6 | 57 | 4 | 38 | 9.88 | 265.61 | -41.69 | 80.01 | 0.6677 | 1007.7 | 400.3 | |
| 0 | 6 | 0 | 4 | 12.08 | 264.48 | -42.83 | 76.92 | 0.6848 | -807.0 | -716.1 | |
| 0 | 4 | 0 | 3 | 10.96 | 263.78 | -43.53 | 78.66 | 0.6920 | -547.0 | -539.9 | |
| 0 | 5 | 0 | 3 | 12.00 | 263.52 | -43.79 | 77.20 | 0.6965 | -671.0 | -596.8 | |
| 0 | 9 | 0 | 7 | 13.23 | 262.31 | -45.00 | 75.66 | 0.7129 | -692.0 | -550.2 | |
| 0 | 3 | 0 | 2 | 13.92 | 259.12 | -48.19 | 75.22 | 0.7506 | -566.0 | -485.5 | |
| 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. | |