SOHO MDI 2000-11-01 18:01:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74 | 542 | 44 | 313 | -23.47 | 306.12 | 14.86 | 206.97 | 0.5213 | -1161.8 | -588.2 | |
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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 | -25.90 | 313.79 | 22.53 | 214.76 | 0.6070 | -421.0 | -320.0 | |
| 0 | 4 | 0 | 2 | -21.03 | 310.50 | 19.25 | 216.05 | 0.5250 | -614.0 | -573.2 | |
| 0 | 4 | 0 | 2 | -23.21 | 310.11 | 18.85 | 213.01 | 0.5472 | -533.0 | -536.0 | |
| 0 | 10 | 0 | 5 | -18.19 | 307.72 | 16.47 | 215.45 | 0.4663 | 807.0 | 597.2 | |
| 6 | 13 | 3 | 8 | -23.38 | 308.19 | 16.93 | 210.15 | 0.5345 | -675.7 | -462.1 | |
| 19 | 133 | 11 | 77 | -22.46 | 307.33 | 16.08 | 209.83 | 0.5165 | -1602.0 | -692.7 | |
| 0 | 8 | 0 | 5 | -24.92 | 306.63 | 15.38 | 206.39 | 0.5431 | -697.0 | -564.8 | |
| 4 | 11 | 3 | 6 | -22.56 | 306.05 | 14.79 | 207.74 | 0.5085 | -1165.4 | -915.8 | |
| 0 | 9 | 0 | 5 | -25.09 | 306.13 | 14.87 | 205.50 | 0.5420 | -783.0 | -558.2 | |
| 23 | 290 | 14 | 168 | -23.89 | 305.63 | 14.38 | 205.82 | 0.5233 | -1364.7 | -675.2 | |
| 4 | 40 | 3 | 24 | -25.34 | 305.28 | 14.02 | 204.02 | 0.5400 | -212.0 | -26.5 | |
| 15 | -10 | 8 | -10 | -23.49 | 305.07 | 13.81 | 205.31 | 0.5143 | -1409.8 | 999999 | |
| -12 | -10 | -12 | -10 | -23.75 | 304.84 | 13.58 | 204.71 | 0.5162 | 999999 | 999999 | |
| 3 | -11 | 2 | -11 | -25.64 | 304.92 | 13.66 | 203.23 | 0.5419 | 867.6 | 999999 | |
| 0 | 6 | 0 | 3 | -21.22 | 303.15 | 11.89 | 204.16 | 0.4711 | -734.0 | -661.2 | |
| 0 | 7 | 0 | 4 | -22.16 | 303.18 | 11.93 | 203.37 | 0.4844 | 245.0 | 153.2 | |
| 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. | |