SOHO MDI 2000-11-03 01:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 81 | 503 | 41 | 259 | -10.29 | 277.12 | 3.19 | 193.55 | 0.2661 | -1084.8 | -384.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45 | 303 | 23 | 155 | -9.37 | 279.92 | 5.99 | 203.91 | 0.2553 | -1963.8 | -686.9 | |
| 18 | 63 | 9 | 32 | -9.80 | 278.24 | 4.31 | 197.18 | 0.2520 | -1339.0 | -655.1 | |
| 0 | 5 | 0 | 3 | -8.73 | 277.25 | 3.32 | 194.50 | 0.2299 | -735.0 | -589.7 | |
| 0 | 7 | 0 | 3 | -8.69 | 276.86 | 2.93 | 192.90 | 0.2276 | -740.0 | -608.4 | |
| 0 | 5 | 0 | 3 | -10.27 | 275.97 | 2.05 | 188.08 | 0.2514 | 476.0 | 364.2 | |
| 0 | 7 | 0 | 4 | -10.90 | 274.29 | 0.37 | 181.39 | 0.2598 | -729.0 | -663.1 | |
| 0 | 6 | 0 | 3 | -14.60 | 273.86 | -0.07 | 179.80 | 0.3217 | -546.0 | -450.5 | |
| 2 | 7 | 1 | 4 | -12.87 | 270.54 | -3.38 | 168.84 | 0.2984 | -534.8 | -388.1 | |
| 0 | 7 | 0 | 4 | -13.88 | 270.29 | -3.63 | 168.71 | 0.3157 | -1149.0 | -843.9 | |
| 0 | 5 | 0 | 3 | -13.19 | 269.94 | -3.98 | 167.17 | 0.3058 | 1004.0 | 783.3 | |
| 0 | 8 | 0 | 4 | -16.45 | 269.76 | -4.16 | 168.77 | 0.3590 | -1086.0 | -874.3 | |
| 6 | 41 | 3 | 21 | -11.71 | 269.61 | -4.31 | 164.85 | 0.2830 | 1428.6 | 1066.2 | |
| 0 | 10 | 0 | 5 | -13.44 | 269.54 | -4.38 | 166.13 | 0.3113 | 1213.0 | 852.8 | |
| 6 | -12 | 3 | -12 | -11.63 | 269.34 | -4.59 | 163.86 | 0.2830 | 1564.0 | 999999 | |
| 0 | 4 | 0 | 2 | -14.50 | 268.13 | -5.80 | 162.92 | 0.3345 | 585.0 | 476.4 | |
| 4 | 25 | 2 | 13 | -13.53 | 267.63 | -6.29 | 160.58 | 0.3218 | 1234.3 | 993.0 | |
| 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. | |