SOHO MDI 2000-07-13 19:11:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67 | 474 | 114 | 1145 | -18.35 | 32.75 | 75.92 | 250.10 | 0.9744 | 409.6 | 28.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 92 | 0 | 477 | -18.38 | 39.61 | 82.78 | 251.04 | 0.9959 | 84.0 | 31.0 | |
| 0 | 2 | 0 | 6 | -16.58 | 35.71 | 78.88 | 252.40 | 0.9874 | -281.0 | -209.1 | |
| 0 | 5 | 0 | 16 | -18.07 | 36.65 | 79.82 | 251.01 | 0.9902 | -295.0 | -273.0 | |
| 0 | 11 | 0 | 28 | -16.77 | 33.21 | 76.38 | 251.88 | 0.9800 | -403.0 | -378.3 | |
| 0 | 1 | 0 | 2 | -16.97 | 29.21 | 72.38 | 251.06 | 0.9649 | -280.0 | -383.7 | |
| 7 | 62 | 11 | 96 | -15.69 | 25.96 | 69.13 | 251.82 | 0.9482 | 661.9 | 325.0 | |
| 0 | 5 | 0 | 9 | -16.58 | 26.65 | 69.82 | 251.03 | 0.9526 | 96.0 | 124.0 | |
| 11 | 188 | 21 | 347 | -18.77 | 28.42 | 71.59 | 249.09 | 0.9629 | 206.2 | -141.3 | |
| 3 | -6 | 4 | -6 | -15.96 | 25.70 | 68.87 | 251.49 | 0.9471 | 616.3 | 999999 | |
| 13 | -8 | 24 | -8 | -19.57 | 28.87 | 72.04 | 248.35 | 0.9655 | 260.4 | 999999 | |
| 7 | -8 | 14 | -8 | -20.04 | 28.85 | 72.02 | 247.87 | 0.9658 | 260.2 | 999999 | |
| 5 | 38 | 8 | 56 | -16.95 | 24.85 | 68.02 | 250.30 | 0.9436 | 692.1 | 387.2 | |
| 13 | 70 | 20 | 108 | -18.41 | 25.24 | 68.41 | 248.86 | 0.9473 | 551.9 | 273.4 | |
| 8 | -13 | 12 | -13 | -18.94 | 25.46 | 68.63 | 248.36 | 0.9490 | 571.2 | 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. | |