SOHO MDI 2000-11-01 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 98 | 752 | 50 | 391 | 2.66 | 271.81 | -17.04 | 94.70 | 0.2952 | 1765.8 | 684.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32 | 697 | 16 | 360 | 2.23 | 272.97 | -15.89 | 96.58 | 0.2767 | 2206.7 | 711.9 | |
| 14 | -1 | 7 | -1 | 2.18 | 272.49 | -16.37 | 96.53 | 0.2848 | 1680.3 | 999999 | |
| 15 | -1 | 8 | -1 | 3.40 | 272.07 | -16.79 | 92.13 | 0.2899 | 1575.4 | 999999 | |
| 0 | 6 | 0 | 3 | 0.82 | 272.06 | -16.80 | 100.92 | 0.2957 | 855.0 | 675.6 | |
| 26 | -1 | 13 | -1 | 2.82 | 271.59 | -17.26 | 94.02 | 0.2985 | 1811.0 | 999999 | |
| 4 | -1 | 2 | -1 | 3.32 | 271.55 | -17.31 | 92.33 | 0.2987 | 1327.4 | 999999 | |
| 0 | 7 | 0 | 3 | 0.50 | 271.57 | -17.28 | 101.62 | 0.3047 | 701.0 | 517.9 | |
| 7 | -1 | 4 | -1 | 2.89 | 271.23 | -17.63 | 93.68 | 0.3045 | 1289.7 | 999999 | |
| 0 | 5 | 0 | 3 | 4.34 | 271.00 | -17.86 | 88.87 | 0.3073 | 390.0 | 472.3 | |
| 0 | 3 | 0 | 2 | 4.42 | 269.45 | -19.41 | 88.60 | 0.3330 | 584.0 | 461.6 | |
| 0 | 9 | 0 | 5 | 3.24 | 266.92 | -21.94 | 91.75 | 0.3749 | 824.0 | 702.1 | |
| 0 | 7 | 0 | 4 | 0.69 | 266.70 | -22.16 | 98.41 | 0.3829 | 842.0 | 674.0 | |
| 0 | 5 | 0 | 3 | 4.77 | 266.42 | -22.44 | 87.67 | 0.3824 | -883.0 | -704.3 | |
| 0 | 4 | 0 | 2 | 2.34 | 266.44 | -22.42 | 94.03 | 0.3837 | 575.0 | 659.8 | |
| 0 | 5 | 0 | 3 | 1.37 | 263.58 | -25.28 | 95.66 | 0.4308 | 668.0 | 494.1 | |
| 0 | 4 | 0 | 3 | 5.40 | 259.59 | -29.27 | 86.44 | 0.4897 | -603.0 | -485.8 | |
| 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. | |