SOHO MDI 2000-11-01 14:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79 | 272 | 55 | 188 | 19.34 | 250.19 | -43.06 | 66.54 | 0.7041 | 99.6 | -86.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16 | 162 | 11 | 109 | 18.83 | 252.46 | -40.79 | 66.49 | 0.6767 | 1016.7 | 248.6 | |
| 6 | -1 | 4 | -1 | 19.34 | 252.09 | -41.16 | 65.90 | 0.6827 | 427.1 | 999999 | |
| -1 | -1 | -1 | -1 | 18.47 | 252.35 | -40.90 | 67.05 | 0.6767 | 999999 | 999999 | |
| 17 | -1 | 11 | -1 | 19.35 | 251.54 | -41.71 | 66.08 | 0.6891 | 604.5 | 999999 | |
| 10 | -1 | 6 | -1 | 18.24 | 251.77 | -41.48 | 67.57 | 0.6829 | 806.5 | 999999 | |
| 3 | -1 | 2 | -1 | 19.60 | 250.91 | -42.34 | 65.95 | 0.6972 | 212.4 | 999999 | |
| 0 | 7 | 0 | 5 | 20.23 | 250.53 | -42.72 | 65.21 | 0.7035 | -572.0 | -514.1 | |
| 0 | 7 | 0 | 5 | 19.10 | 249.62 | -43.63 | 67.07 | 0.7103 | -336.0 | -321.6 | |
| 0 | 5 | 0 | 3 | 17.69 | 249.40 | -43.86 | 69.09 | 0.7090 | 364.0 | 175.1 | |
| 0 | 4 | 0 | 3 | 18.27 | 249.04 | -44.21 | 68.39 | 0.7146 | 203.0 | 95.9 | |
| 1 | 8 | 1 | 5 | 19.48 | 248.46 | -44.79 | 66.91 | 0.7244 | -712.0 | -582.3 | |
| 0 | 4 | 0 | 3 | 19.04 | 248.44 | -44.81 | 67.51 | 0.7234 | -526.0 | -396.8 | |
| 9 | 64 | 7 | 47 | 20.61 | 247.64 | -45.62 | 65.65 | 0.7366 | -1054.5 | -666.5 | |
| 0 | 3 | 0 | 2 | 19.80 | 247.59 | -45.66 | 66.74 | 0.7349 | -387.0 | -456.0 | |
| 17 | -13 | 13 | -13 | 20.25 | 247.00 | -46.25 | 66.31 | 0.7424 | -822.7 | 999999 | |
| 0 | 8 | 0 | 6 | 19.16 | 246.82 | -46.43 | 67.81 | 0.7415 | -749.0 | -609.3 | |
| 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. | |