SOHO MDI 2000-09-27 11:11:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42 | 173 | 32 | 133 | -12.01 | 349.18 | -47.28 | 111.78 | 0.7744 | 160.2 | 120.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -10.52 | 357.48 | -38.98 | 113.77 | 0.6781 | -461.0 | -308.2 | |
| 6 | 12 | 4 | 9 | -11.90 | 356.59 | -39.87 | 115.13 | 0.6952 | -906.0 | -652.1 | |
| 9 | 21 | 6 | 14 | -11.53 | 356.13 | -40.33 | 114.38 | 0.6986 | -892.2 | -578.3 | |
| 0 | 7 | 0 | 5 | -11.43 | 352.82 | -43.64 | 112.58 | 0.7349 | -754.0 | -612.0 | |
| 0 | 4 | 0 | 3 | -11.56 | 350.37 | -46.09 | 111.64 | 0.7616 | 612.0 | 413.2 | |
| 0 | 6 | 0 | 4 | -13.41 | 349.47 | -46.99 | 113.50 | 0.7779 | -429.0 | -394.9 | |
| 0 | 7 | 0 | 5 | -13.61 | 349.00 | -47.46 | 113.55 | 0.7834 | -624.0 | -439.6 | |
| 0 | 2 | 0 | 1 | -10.56 | 348.84 | -47.62 | 109.77 | 0.7740 | 483.0 | 483.0 | |
| 0 | 6 | 0 | 5 | -14.12 | 347.59 | -48.86 | 113.54 | 0.7990 | 659.0 | 496.3 | |
| 6 | 22 | 5 | 18 | -10.87 | 347.76 | -48.70 | 109.72 | 0.7861 | 701.9 | 791.5 | |
| 0 | 3 | 0 | 2 | -10.24 | 347.53 | -48.93 | 108.87 | 0.7863 | 441.0 | 367.3 | |
| 0 | 4 | 0 | 3 | -12.36 | 347.03 | -49.43 | 111.23 | 0.7983 | 495.0 | 444.9 | |
| 8 | 31 | 7 | 26 | -13.63 | 346.62 | -49.84 | 112.57 | 0.8065 | 649.8 | 405.2 | |
| 11 | 36 | 9 | 29 | -11.42 | 346.65 | -49.81 | 109.96 | 0.7989 | 643.4 | 144.6 | |
| 2 | 9 | 1 | 7 | -10.62 | 346.46 | -49.99 | 108.94 | 0.7982 | 458.2 | 316.7 | |
| 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. | |