SOHO MDI 2000-11-01 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 66 | 237 | 47 | 168 | 19.33 | 250.03 | -44.10 | 66.89 | 0.7159 | 139.8 | -186.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6 | 110 | 4 | 75 | 18.83 | 252.36 | -41.77 | 66.84 | 0.6881 | 863.6 | 18.7 | |
| 9 | -1 | 6 | -1 | 18.51 | 252.30 | -41.83 | 67.32 | 0.6879 | 967.5 | 999999 | |
| 9 | -1 | 6 | -1 | 19.33 | 251.88 | -42.25 | 66.31 | 0.6953 | 73.5 | 999999 | |
| 13 | -1 | 9 | -1 | 19.38 | 251.36 | -42.77 | 66.40 | 0.7014 | 593.2 | 999999 | |
| 7 | 24 | 5 | 17 | 18.27 | 251.60 | -42.53 | 67.88 | 0.6953 | 693.7 | 467.1 | |
| 4 | -1 | 3 | -1 | 19.64 | 250.82 | -43.31 | 66.23 | 0.7083 | 145.6 | 999999 | |
| 0 | 10 | 0 | 7 | 20.23 | 250.62 | -43.51 | 65.48 | 0.7124 | -707.0 | -551.0 | |
| 0 | 7 | 0 | 5 | 17.73 | 249.41 | -44.72 | 69.28 | 0.7190 | 72.0 | 267.0 | |
| 2 | 13 | 2 | 9 | 19.49 | 248.58 | -45.55 | 67.13 | 0.7328 | -743.5 | -615.2 | |
| 0 | 6 | 0 | 4 | 18.30 | 248.88 | -45.25 | 68.64 | 0.7264 | 23.0 | 34.1 | |
| 0 | 3 | 0 | 3 | 19.08 | 248.43 | -45.70 | 67.72 | 0.7333 | -363.0 | -444.8 | |
| 4 | 18 | 3 | 13 | 20.57 | 247.69 | -46.44 | 65.95 | 0.7453 | -1034.8 | -816.6 | |
| 12 | 36 | 9 | 27 | 20.22 | 247.05 | -47.08 | 66.60 | 0.7511 | -817.0 | -594.9 | |
| 0 | 10 | 0 | 8 | 19.16 | 246.98 | -47.15 | 68.00 | 0.7493 | -471.0 | -581.4 | |
| 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. | |