SOHO MDI 2000-07-08 15:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 105 | 628 | 196 | 1140 | 18.45 | 310.33 | -74.46 | 71.81 | 0.9595 | -254.8 | -172.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13 | 68 | 13 | 72 | 18.86 | 323.37 | -61.43 | 70.59 | 0.8830 | 800.0 | 336.9 | |
| 2 | 14 | 3 | 16 | 18.34 | 320.08 | -64.71 | 71.49 | 0.9068 | 263.9 | 8.3 | |
| 0 | 5 | 0 | 6 | 18.52 | 318.74 | -66.05 | 71.41 | 0.9161 | -206.0 | -258.5 | |
| 5 | 133 | 7 | 179 | 19.19 | 317.45 | -67.34 | 70.77 | 0.9247 | -643.6 | -255.2 | |
| 0 | 4 | 0 | 5 | 17.20 | 317.50 | -67.29 | 72.92 | 0.9236 | -503.0 | -464.9 | |
| 12 | -4 | 16 | -4 | 18.81 | 315.96 | -68.83 | 71.27 | 0.9336 | -327.8 | 999999 | |
| 0 | 2 | 0 | 3 | 17.33 | 316.17 | -68.62 | 72.85 | 0.9319 | -339.0 | -341.2 | |
| 9 | 402 | 16 | 859 | 19.02 | 310.50 | -74.30 | 71.28 | 0.9622 | -386.8 | -198.3 | |
| 6 | -8 | 12 | -8 | 19.13 | 308.86 | -75.93 | 71.21 | 0.9692 | -168.1 | 999999 | |
| 18 | -8 | 38 | -8 | 18.55 | 308.25 | -76.55 | 71.82 | 0.9716 | -592.8 | 999999 | |
| 4 | -8 | 11 | -8 | 19.73 | 305.70 | -79.10 | 70.62 | 0.9807 | 133.0 | 999999 | |
| 7 | -8 | 15 | -8 | 17.60 | 308.46 | -76.33 | 72.79 | 0.9707 | -546.5 | 999999 | |
| 5 | -8 | 12 | -8 | 19.33 | 305.31 | -79.48 | 71.03 | 0.9819 | 10.7 | 999999 | |
| 10 | -8 | 25 | -8 | 18.55 | 305.60 | -79.19 | 71.83 | 0.9810 | -320.7 | 999999 | |
| 8 | -8 | 17 | -8 | 16.69 | 307.83 | -76.96 | 73.73 | 0.9732 | -144.2 | 999999 | |
| 6 | -8 | 11 | -8 | 16.13 | 308.18 | -76.62 | 74.30 | 0.9718 | -319.6 | 999999 | |
| 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. | |