SOHO MDI 2000-11-03 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 100 | 468 | 65 | 310 | -23.17 | 304.93 | 31.88 | 227.25 | 0.6629 | -861.3 | -344.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23 | 84 | 15 | 57 | -22.53 | 307.55 | 34.51 | 230.18 | 0.6836 | -1125.3 | -543.5 | |
| 0 | 3 | 0 | 2 | -19.61 | 306.79 | 33.74 | 233.27 | 0.6552 | 432.0 | 354.0 | |
| 24 | 212 | 16 | 142 | -24.11 | 306.04 | 32.99 | 227.11 | 0.6808 | -1054.4 | -338.1 | |
| -3 | -3 | -3 | -3 | -24.26 | 305.63 | 32.59 | 226.59 | 0.6782 | 999999 | 999999 | |
| 10 | -3 | 6 | -3 | -23.82 | 305.41 | 32.36 | 226.93 | 0.6726 | -1299.3 | 999999 | |
| 9 | -3 | 6 | -3 | -23.54 | 305.03 | 31.98 | 226.95 | 0.6669 | -1283.8 | 999999 | |
| 0 | 1 | 0 | 1 | -20.03 | 303.64 | 30.59 | 230.14 | 0.6252 | -451.0 | -505.9 | |
| 0 | 3 | 0 | 2 | -24.27 | 304.64 | 31.59 | 225.76 | 0.6690 | -578.0 | -587.6 | |
| 0 | 14 | 0 | 9 | -25.06 | 304.81 | 31.77 | 224.98 | 0.6770 | -325.0 | -353.2 | |
| 3 | 7 | 2 | 4 | -23.13 | 304.28 | 31.23 | 226.81 | 0.6564 | -788.7 | -730.2 | |
| 13 | 49 | 8 | 31 | -20.45 | 303.44 | 30.40 | 229.43 | 0.6264 | -1105.0 | -734.1 | |
| 0 | 5 | 0 | 3 | -21.47 | 303.58 | 30.53 | 228.25 | 0.6361 | 75.0 | 138.7 | |
| 4 | 34 | 3 | 22 | -22.80 | 303.61 | 30.56 | 226.63 | 0.6472 | -1105.3 | -688.5 | |
| 2 | -13 | 2 | -13 | -22.91 | 303.10 | 30.06 | 226.04 | 0.6433 | -377.9 | 999999 | |
| 0 | 5 | 0 | 4 | -24.66 | 303.51 | 30.46 | 224.32 | 0.6618 | -436.0 | -363.5 | |
| 5 | 16 | 3 | 11 | -25.57 | 303.27 | 30.22 | 223.05 | 0.6674 | 777.0 | 458.7 | |
| 0 | 4 | 0 | 3 | -22.51 | 300.49 | 27.44 | 224.04 | 0.6146 | 523.0 | 500.8 | |
| 7 | 26 | 4 | 16 | -22.40 | 299.81 | 26.76 | 223.49 | 0.6071 | 1035.6 | 679.2 | |
| 0 | 5 | 0 | 3 | -20.49 | 292.68 | 19.63 | 217.39 | 0.5204 | 274.0 | 312.2 | |
| 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. | |