SOHO MDI 2000-11-02 17:51:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 103 | 797 | 51 | 397 | 2.71 | 271.55 | -6.62 | 103.34 | 0.1192 | 1860.1 | 664.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26 | 693 | 13 | 345 | 2.21 | 273.12 | -5.05 | 110.52 | 0.0943 | 2213.3 | 761.4 | |
| 27 | -1 | 13 | -1 | 2.13 | 272.58 | -5.59 | 109.39 | 0.1036 | 1982.4 | 999999 | |
| 6 | -1 | 3 | -1 | 3.28 | 272.31 | -5.86 | 97.87 | 0.1035 | 1725.8 | 999999 | |
| 4 | -1 | 2 | -1 | 2.55 | 272.20 | -5.98 | 104.48 | 0.1079 | 1611.2 | 999999 | |
| 0 | 4 | 0 | 2 | 4.01 | 271.91 | -6.26 | 90.71 | 0.1092 | 659.0 | 612.6 | |
| 34 | -1 | 17 | -1 | 2.90 | 271.77 | -6.40 | 100.59 | 0.1139 | 1976.8 | 999999 | |
| 6 | -1 | 3 | -1 | 3.51 | 271.57 | -6.60 | 95.02 | 0.1157 | 1238.6 | 999999 | |
| 0 | 6 | 0 | 3 | 4.28 | 271.56 | -6.61 | 88.33 | 0.1153 | 517.0 | 520.8 | |
| 0 | 5 | 0 | 2 | 0.24 | 271.43 | -6.74 | 119.76 | 0.1359 | 645.0 | 462.2 | |
| 0 | 10 | 0 | 5 | 4.70 | 271.36 | -6.81 | 84.80 | 0.1192 | 670.0 | 505.5 | |
| 0 | 6 | 0 | 3 | 2.99 | 269.59 | -8.58 | 97.19 | 0.1509 | 522.0 | 376.3 | |
| 0 | 4 | 0 | 2 | 3.54 | 267.28 | -10.89 | 92.65 | 0.1897 | 457.0 | 442.7 | |
| 0 | 16 | 0 | 8 | 2.03 | 266.51 | -11.66 | 99.81 | 0.2060 | 825.0 | 716.2 | |
| 0 | 3 | 0 | 2 | 1.45 | 266.51 | -11.66 | 102.55 | 0.2080 | 813.0 | 811.8 | |
| 0 | 4 | 0 | 2 | 2.56 | 266.27 | -11.91 | 97.06 | 0.2086 | 795.0 | 731.3 | |
| 0 | 9 | 0 | 5 | 5.26 | 264.28 | -13.89 | 84.70 | 0.2411 | -1070.0 | -773.4 | |
| 0 | 5 | 0 | 2 | 6.19 | 264.22 | -13.95 | 80.93 | 0.2438 | -830.0 | -690.2 | |
| 0 | 14 | 0 | 7 | 6.44 | 263.29 | -14.88 | 80.44 | 0.2599 | -791.0 | -725.3 | |
| 0 | 8 | 0 | 4 | 2.63 | 263.37 | -14.80 | 95.26 | 0.2574 | -712.0 | -590.0 | |
| 0 | 5 | 0 | 2 | 1.66 | 259.24 | -18.93 | 96.85 | 0.3281 | -856.0 | -798.2 | |
| 0 | 5 | 0 | 3 | 2.43 | 259.19 | -18.98 | 94.49 | 0.3275 | -731.0 | -583.0 | |
| 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. | |