SOHO MDI 2000-10-04 19:25:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 63 | 583 | 36 | 331 | -8.93 | 323.79 | 24.19 | 237.13 | 0.4827 | -1616.8 | -451.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58 | 436 | 33 | 250 | -8.89 | 325.77 | 26.18 | 239.79 | 0.5064 | -1849.7 | -609.9 | |
| 5 | 12 | 3 | 7 | -8.05 | 324.10 | 24.51 | 239.61 | 0.4781 | -1087.7 | -825.7 | |
| 0 | 5 | 0 | 3 | -7.41 | 322.39 | 22.80 | 238.95 | 0.4504 | -849.0 | -789.1 | |
| 0 | 5 | 0 | 3 | -8.20 | 321.29 | 21.70 | 236.14 | 0.4426 | -803.0 | -771.0 | |
| 0 | 13 | 0 | 7 | -9.65 | 321.30 | 21.71 | 233.48 | 0.4556 | -885.0 | -696.0 | |
| 0 | 4 | 0 | 2 | -7.79 | 321.06 | 21.47 | 236.63 | 0.4360 | -906.0 | -790.5 | |
| 0 | 6 | 0 | 3 | -8.01 | 320.69 | 21.10 | 235.73 | 0.4332 | -984.0 | -917.2 | |
| 0 | 11 | 0 | 6 | -9.49 | 320.44 | 20.85 | 232.65 | 0.4435 | -739.0 | -774.3 | |
| 0 | 5 | 0 | 3 | -5.24 | 320.07 | 20.47 | 240.62 | 0.4014 | -894.0 | -772.3 | |
| 0 | 7 | 0 | 4 | -4.43 | 319.79 | 20.20 | 242.07 | 0.3913 | -853.0 | -647.2 | |
| 0 | 5 | 0 | 3 | -8.66 | 316.61 | 17.02 | 228.45 | 0.3883 | 482.0 | 446.6 | |
| 0 | 10 | 0 | 6 | -8.68 | 315.91 | 16.32 | 227.22 | 0.3801 | 617.0 | 553.3 | |
| 0 | 7 | 0 | 4 | -7.74 | 315.47 | 15.87 | 228.30 | 0.3646 | 891.0 | 713.9 | |
| 0 | 19 | 0 | 10 | -7.44 | 314.97 | 15.37 | 228.00 | 0.3553 | 1165.0 | 1013.2 | |
| 0 | 9 | 0 | 5 | -14.11 | 314.82 | 15.23 | 216.22 | 0.4331 | 841.0 | 662.6 | |
| 0 | 5 | 0 | 2 | -13.31 | 314.48 | 14.89 | 216.73 | 0.4198 | 944.0 | 770.6 | |
| 0 | 5 | 0 | 3 | -12.57 | 313.04 | 13.45 | 215.05 | 0.3969 | 991.0 | 834.8 | |
| 0 | 6 | 0 | 3 | -12.55 | 312.26 | 12.67 | 213.50 | 0.3896 | 820.0 | 794.9 | |
| 0 | 6 | 0 | 3 | -12.95 | 311.92 | 12.32 | 212.20 | 0.3920 | 616.0 | 565.0 | |
| 0 | 7 | 0 | 4 | -9.71 | 310.97 | 11.38 | 215.09 | 0.3397 | 929.0 | 812.7 | |
| 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. | |