SOHO MDI 2000-11-01 08:40:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 107 | 0 | 60 | -27.19 | 292.50 | -3.89 | 173.38 | 0.5275 | 765.0 | 729.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 3 | -28.64 | 295.28 | -1.11 | 178.20 | 0.5455 | 693.0 | 659.4 | |
| 0 | 4 | 0 | 2 | -26.95 | 294.90 | -1.49 | 177.45 | 0.5208 | 559.0 | 509.0 | |
| 0 | 4 | 0 | 2 | -29.19 | 294.87 | -1.52 | 177.60 | 0.5538 | 592.0 | 456.9 | |
| 0 | 3 | 0 | 2 | -29.52 | 294.20 | -2.19 | 176.58 | 0.5590 | 510.0 | 494.1 | |
| 0 | 3 | 0 | 2 | -27.54 | 293.51 | -2.89 | 175.16 | 0.5309 | 613.0 | 502.7 | |
| 0 | 4 | 0 | 2 | -25.66 | 293.34 | -3.05 | 174.50 | 0.5030 | 788.0 | 550.8 | |
| 0 | 15 | 0 | 8 | -26.87 | 293.22 | -3.17 | 174.55 | 0.5213 | 1004.0 | 773.6 | |
| 0 | 7 | 0 | 4 | -25.17 | 292.71 | -3.68 | 173.26 | 0.4967 | 757.0 | 764.5 | |
| 0 | 11 | 0 | 6 | -26.56 | 292.58 | -3.81 | 173.38 | 0.5176 | 1268.0 | 1027.4 | |
| 0 | 6 | 0 | 3 | -29.71 | 292.47 | -3.92 | 173.93 | 0.5639 | 681.0 | 605.5 | |
| 0 | 14 | 0 | 8 | -26.56 | 292.15 | -4.24 | 172.64 | 0.5185 | 1241.0 | 1034.8 | |
| 0 | 6 | 0 | 3 | -26.70 | 291.50 | -4.89 | 171.57 | 0.5219 | 949.0 | 772.2 | |
| 0 | 12 | 0 | 7 | -27.78 | 291.32 | -5.07 | 171.61 | 0.5382 | 680.0 | 644.6 | |
| 0 | 5 | 0 | 3 | -27.20 | 290.87 | -5.52 | 170.68 | 0.5306 | 558.0 | 516.8 | |
| 0 | 5 | 0 | 3 | -27.02 | 290.09 | -6.30 | 169.33 | 0.5301 | 703.0 | 607.4 | |
| 0 | 4 | 0 | 2 | -26.89 | 289.58 | -6.81 | 168.43 | 0.5297 | 644.0 | 517.9 | |
| 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. | |