SOHO MDI 2000-11-03 19:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59 | 424 | 31 | 224 | -9.83 | 278.52 | 14.26 | 225.24 | 0.3457 | -1773.6 | -540.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 5 | 0 | 2 | -6.13 | 280.44 | 16.18 | 237.99 | 0.3282 | -808.0 | -704.9 | |
| 0 | 4 | 0 | 2 | -11.73 | 280.25 | 15.99 | 225.12 | 0.3823 | 334.0 | 418.9 | |
| 49 | 280 | 26 | 148 | -9.30 | 280.04 | 15.78 | 229.70 | 0.3534 | -1989.4 | -642.7 | |
| 10 | 54 | 5 | 29 | -9.79 | 278.73 | 14.47 | 226.17 | 0.3428 | -1483.9 | -823.6 | |
| 0 | 10 | 0 | 5 | -10.55 | 278.64 | 14.38 | 224.43 | 0.3503 | -413.0 | -410.3 | |
| 0 | 10 | 0 | 5 | -7.80 | 277.73 | 13.47 | 228.70 | 0.3085 | -776.0 | -708.5 | |
| 0 | 11 | 0 | 6 | -8.55 | 277.47 | 13.21 | 226.37 | 0.3137 | -999.0 | -807.5 | |
| 0 | 5 | 0 | 3 | -14.14 | 275.55 | 11.29 | 211.46 | 0.3652 | -927.0 | -805.6 | |
| 0 | 4 | 0 | 2 | -10.15 | 273.55 | 9.29 | 213.11 | 0.2922 | -534.0 | -425.9 | |
| 0 | 9 | 0 | 5 | -16.70 | 269.92 | 5.66 | 194.97 | 0.3672 | -611.0 | -517.5 | |
| 0 | 6 | 0 | 3 | -13.44 | 269.64 | 5.37 | 196.92 | 0.3144 | 1022.0 | 909.0 | |
| 0 | 8 | 0 | 4 | -11.83 | 269.60 | 5.34 | 198.48 | 0.2887 | 1134.0 | 802.7 | |
| 0 | 7 | 0 | 4 | -11.75 | 269.20 | 4.94 | 197.28 | 0.2853 | 1004.0 | 892.2 | |
| 0 | 11 | 0 | 6 | -13.59 | 267.38 | 3.11 | 189.91 | 0.3080 | 1110.0 | 896.6 | |
| 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. | |