SOHO MDI 2000-07-03 19:11:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 100 | 557 | 72 | 392 | -19.08 | 49.03 | -40.20 | 121.13 | 0.7129 | -659.3 | -162.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41 | 266 | 28 | 178 | -18.07 | 52.30 | -36.93 | 121.70 | 0.6737 | -1481.8 | -635.6 | |
| 6 | 30 | 4 | 21 | -19.03 | 51.74 | -37.49 | 122.61 | 0.6853 | -735.9 | -282.8 | |
| -1 | -1 | -1 | -1 | -17.74 | 52.01 | -37.22 | 121.08 | 0.6750 | 999999 | 999999 | |
| 11 | -1 | 8 | -1 | -18.10 | 51.50 | -37.73 | 121.24 | 0.6826 | -868.3 | 999999 | |
| 0 | 3 | 0 | 2 | -18.80 | 51.05 | -38.17 | 121.88 | 0.6913 | -293.0 | -306.0 | |
| 3 | 36 | 2 | 25 | -18.35 | 50.48 | -38.75 | 120.95 | 0.6951 | -413.0 | -5.6 | |
| 0 | 5 | 0 | 3 | -16.18 | 50.91 | -38.32 | 118.33 | 0.6788 | -549.0 | -473.7 | |
| 0 | 7 | 0 | 4 | -17.12 | 50.47 | -38.75 | 119.34 | 0.6886 | -361.0 | -275.9 | |
| 0 | 5 | 0 | 3 | -19.06 | 49.69 | -39.54 | 121.41 | 0.7073 | -283.0 | -295.7 | |
| 13 | 54 | 10 | 40 | -21.36 | 46.87 | -42.36 | 122.70 | 0.7479 | -879.9 | -320.8 | |
| 4 | -10 | 3 | -10 | -20.84 | 47.00 | -42.23 | 122.13 | 0.7440 | -531.1 | 999999 | |
| 0 | 2 | 0 | 2 | -22.10 | 45.90 | -43.33 | 123.06 | 0.7609 | -130.0 | -100.1 | |
| 1 | 7 | 1 | 5 | -22.76 | 44.61 | -44.61 | 123.19 | 0.7761 | 629.8 | 512.5 | |
| 6 | 82 | 4 | 62 | -19.70 | 45.48 | -43.75 | 119.95 | 0.7536 | 1174.0 | 684.2 | |
| 4 | -14 | 3 | -14 | -19.54 | 45.07 | -44.16 | 119.56 | 0.7571 | 839.8 | 999999 | |
| 0 | 4 | 0 | 3 | -20.59 | 44.69 | -44.54 | 120.64 | 0.7654 | 619.0 | 511.0 | |
| 0 | 6 | 0 | 4 | -20.27 | 44.03 | -45.20 | 119.95 | 0.7704 | 740.0 | 614.6 | |
| 5 | 50 | 4 | 40 | -21.24 | 42.61 | -46.62 | 120.44 | 0.7879 | 782.7 | 593.2 | |
| 6 | -18 | 5 | -18 | -21.04 | 42.26 | -46.97 | 120.04 | 0.7904 | 656.6 | 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. | |