SOHO MDI 2000-11-09 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58 | 381 | 31 | 204 | -12.56 | 177.09 | -16.90 | 133.94 | 0.3960 | 1265.3 | 421.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 7 | 0 | 4 | -13.56 | 179.63 | -14.36 | 140.28 | 0.3790 | -683.0 | -551.6 | |
| 0 | 4 | 0 | 2 | -11.02 | 178.76 | -15.23 | 133.80 | 0.3589 | -555.0 | -438.0 | |
| 0 | 3 | 0 | 1 | -12.21 | 178.61 | -15.38 | 135.89 | 0.3741 | 644.0 | 556.3 | |
| 0 | 11 | 0 | 6 | -11.70 | 178.52 | -15.47 | 134.72 | 0.3693 | 774.0 | 468.9 | |
| 19 | 309 | 10 | 166 | -13.39 | 177.80 | -16.19 | 136.60 | 0.3966 | 1141.2 | 621.8 | |
| 24 | -5 | 13 | -5 | -12.43 | 177.49 | -16.50 | 134.32 | 0.3893 | 1842.6 | 999999 | |
| 8 | -5 | 4 | -5 | -12.52 | 176.87 | -17.12 | 133.44 | 0.3975 | 1474.9 | 999999 | |
| 5 | -5 | 3 | -5 | -13.08 | 176.83 | -17.16 | 134.41 | 0.4041 | 940.2 | 999999 | |
| 0 | 6 | 0 | 3 | -9.88 | 176.21 | -17.78 | 127.06 | 0.3786 | -1171.0 | -829.0 | |
| 0 | 6 | 0 | 3 | -15.12 | 173.98 | -20.01 | 133.58 | 0.4580 | -891.0 | -610.9 | |
| 0 | 4 | 0 | 2 | -9.52 | 174.30 | -19.69 | 123.56 | 0.4006 | -676.0 | -642.1 | |
| 0 | 6 | 0 | 3 | -8.93 | 174.12 | -19.87 | 122.08 | 0.3979 | -1003.0 | -844.8 | |
| 0 | 3 | 0 | 2 | -10.67 | 174.01 | -19.98 | 125.56 | 0.4144 | -776.0 | -626.3 | |
| 0 | 5 | 0 | 3 | -10.84 | 173.54 | -20.45 | 125.27 | 0.4220 | -839.0 | -843.7 | |
| 2 | 13 | 1 | 7 | -10.97 | 172.86 | -21.13 | 124.66 | 0.4320 | -906.0 | -623.3 | |
| 0 | 4 | 0 | 2 | -11.46 | 172.32 | -21.67 | 124.93 | 0.4433 | -682.0 | -601.1 | |
| 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. | |