SOHO MDI 2000-07-17 14:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24 | 130 | 18 | 89 | -11.09 | 307.93 | 41.41 | 248.73 | 0.6979 | 103.2 | -76.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4 | 27 | 3 | 20 | -11.05 | 311.60 | 45.08 | 250.41 | 0.7399 | -592.8 | -571.6 | |
| 0 | 2 | 0 | 2 | -10.40 | 310.23 | 43.71 | 250.73 | 0.7223 | -846.0 | -772.7 | |
| 2 | 17 | 2 | 12 | -10.72 | 310.23 | 43.71 | 250.30 | 0.7235 | -884.4 | -808.4 | |
| 2 | -3 | 2 | -3 | -11.00 | 310.12 | 43.60 | 249.88 | 0.7232 | -962.8 | 999999 | |
| 0 | 6 | 0 | 4 | -10.49 | 309.75 | 43.23 | 250.41 | 0.7171 | -645.0 | -504.6 | |
| 0 | 9 | 0 | 6 | -11.40 | 309.80 | 43.28 | 249.23 | 0.7211 | -720.0 | -724.3 | |
| 0 | 3 | 0 | 2 | -11.37 | 309.30 | 42.78 | 249.06 | 0.7152 | -497.0 | -597.3 | |
| 0 | 3 | 0 | 2 | -9.51 | 308.17 | 41.65 | 251.10 | 0.6951 | 133.0 | 250.2 | |
| 4 | 11 | 3 | 7 | -10.18 | 306.25 | 39.73 | 249.31 | 0.6748 | 519.3 | 353.8 | |
| 3 | 17 | 2 | 11 | -10.49 | 305.15 | 38.63 | 248.34 | 0.6628 | 671.8 | 671.0 | |
| 4 | -10 | 3 | -10 | -10.68 | 304.92 | 38.40 | 247.95 | 0.6609 | 875.0 | 999999 | |
| 5 | 16 | 3 | 11 | -12.41 | 304.94 | 38.43 | 245.53 | 0.6692 | 710.0 | 488.7 | |
| 0 | 3 | 0 | 2 | -10.87 | 304.59 | 38.07 | 247.52 | 0.6577 | 227.0 | 422.7 | |
| 0 | 4 | 0 | 2 | -11.61 | 303.94 | 37.42 | 246.10 | 0.6533 | 643.0 | 618.0 | |
| 0 | 12 | 0 | 8 | -11.63 | 303.53 | 37.02 | 245.85 | 0.6485 | 902.0 | 702.3 | |
| 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. | |