SOHO MDI 2000-07-03 17:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 97 | 557 | 70 | 402 | -19.13 | 48.79 | -41.32 | 120.57 | 0.7247 | -529.3 | -152.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13 | 263 | 9 | 179 | -18.15 | 52.32 | -37.79 | 121.26 | 0.6835 | -1238.2 | -657.2 | |
| 22 | -1 | 15 | -1 | -17.73 | 52.05 | -38.06 | 120.55 | 0.6841 | -1560.7 | 999999 | |
| 6 | 35 | 4 | 24 | -19.02 | 51.71 | -38.40 | 122.03 | 0.6949 | -688.4 | -203.6 | |
| 12 | -1 | 8 | -1 | -18.14 | 51.47 | -38.64 | 120.73 | 0.6927 | -877.3 | 999999 | |
| 4 | 26 | 3 | 18 | -18.35 | 50.33 | -39.78 | 120.35 | 0.7060 | -386.6 | 30.1 | |
| 0 | 6 | 0 | 4 | -16.22 | 50.88 | -39.23 | 117.86 | 0.6892 | -594.0 | -521.5 | |
| 0 | 2 | 0 | 2 | -18.78 | 50.05 | -40.06 | 120.75 | 0.7114 | -169.0 | -263.0 | |
| 0 | 4 | 0 | 3 | -19.10 | 49.57 | -40.54 | 120.88 | 0.7180 | -262.0 | -260.6 | |
| 0 | 3 | 0 | 2 | -18.45 | 48.82 | -41.29 | 119.65 | 0.7226 | 359.0 | 325.8 | |
| 12 | 50 | 9 | 38 | -21.40 | 46.81 | -43.30 | 122.24 | 0.7572 | -879.0 | -355.1 | |
| 0 | 5 | 0 | 4 | -22.80 | 44.69 | -45.42 | 122.82 | 0.7836 | 500.0 | 446.1 | |
| 4 | 86 | 3 | 66 | -19.69 | 45.54 | -44.57 | 119.54 | 0.7617 | 1118.7 | 701.8 | |
| 5 | -12 | 4 | -12 | -20.05 | 45.18 | -44.93 | 119.79 | 0.7669 | 540.7 | 999999 | |
| 0 | 11 | 0 | 8 | -18.75 | 45.63 | -44.48 | 118.43 | 0.7567 | 761.0 | 570.0 | |
| 7 | -12 | 5 | -12 | -19.58 | 45.11 | -45.00 | 119.20 | 0.7655 | 608.5 | 999999 | |
| 0 | 9 | 0 | 7 | -20.27 | 44.00 | -46.11 | 119.52 | 0.7791 | 711.0 | 564.1 | |
| 6 | 57 | 5 | 47 | -21.15 | 42.65 | -47.46 | 119.95 | 0.7953 | 797.2 | 429.0 | |
| 6 | -17 | 5 | -17 | -21.08 | 42.24 | -47.87 | 119.69 | 0.7988 | 559.8 | 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. | |