SOHO MDI 2000-11-03 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 125 | 735 | 62 | 365 | 2.64 | 271.46 | 2.80 | 233.89 | 0.0738 | 1849.1 | 655.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41 | 660 | 21 | 328 | 2.14 | 273.07 | 4.42 | 246.88 | 0.0841 | 2049.2 | 744.7 | |
| 18 | -1 | 9 | -1 | 1.95 | 272.65 | 3.99 | 242.50 | 0.0788 | 2034.3 | 999999 | |
| 6 | -1 | 3 | -1 | 3.22 | 272.38 | 3.73 | 257.77 | 0.0667 | 1538.4 | 999999 | |
| 4 | -1 | 2 | -1 | 2.57 | 272.34 | 3.69 | 248.36 | 0.0694 | 1545.2 | 999999 | |
| 7 | -1 | 3 | -1 | 2.26 | 271.95 | 3.30 | 241.79 | 0.0656 | 1518.0 | 999999 | |
| 41 | -1 | 20 | -1 | 2.96 | 271.92 | 3.26 | 251.73 | 0.0601 | 2016.2 | 999999 | |
| -6 | -1 | -6 | -1 | 3.30 | 271.88 | 3.22 | 257.23 | 0.0579 | 999999 | 999999 | |
| 8 | -1 | 4 | -1 | 2.73 | 271.30 | 2.64 | 243.68 | 0.0517 | 1373.7 | 999999 | |
| 0 | 7 | 0 | 3 | 3.39 | 267.95 | -0.71 | 132.73 | 0.0169 | 437.0 | 446.8 | |
| 0 | 6 | 0 | 3 | 3.38 | 266.60 | -2.06 | 107.63 | 0.0378 | 812.0 | 682.3 | |
| 0 | 10 | 0 | 5 | 3.27 | 266.14 | -2.52 | 106.98 | 0.0461 | 868.0 | 678.4 | |
| 0 | 5 | 0 | 2 | 2.34 | 265.10 | -3.56 | 115.45 | 0.0690 | 685.0 | 558.0 | |
| 0 | 5 | 0 | 2 | 1.49 | 264.67 | -3.98 | 122.54 | 0.0827 | 760.0 | 569.5 | |
| 0 | 11 | 0 | 5 | 3.14 | 263.32 | -5.34 | 99.42 | 0.0946 | -872.0 | -704.9 | |
| 0 | 5 | 0 | 3 | 4.41 | 263.19 | -5.46 | 85.93 | 0.0956 | -708.0 | -682.7 | |
| 0 | 5 | 0 | 3 | 4.02 | 263.08 | -5.57 | 89.98 | 0.0974 | -675.0 | -588.4 | |
| 0 | 5 | 0 | 3 | 2.80 | 260.18 | -8.48 | 98.03 | 0.1494 | -773.0 | -626.7 | |
| 0 | 5 | 0 | 3 | 3.64 | 259.27 | -9.38 | 92.12 | 0.1636 | -856.0 | -736.8 | |
| 0 | 4 | 0 | 2 | 4.36 | 258.01 | -10.65 | 87.90 | 0.1852 | -776.0 | -598.5 | |
| 0 | 7 | 0 | 3 | 4.91 | 256.70 | -11.95 | 85.34 | 0.2080 | -588.0 | -479.7 | |
| 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. | |