SOHO MDI 2000-07-03 15:59:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 95 | 514 | 68 | 375 | -19.11 | 48.84 | -42.15 | 120.09 | 0.7332 | -516.7 | -162.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35 | 250 | 24 | 172 | -17.98 | 52.23 | -38.76 | 120.45 | 0.6931 | -1447.9 | -634.5 | |
| 5 | 26 | 3 | 18 | -19.02 | 51.73 | -39.26 | 121.50 | 0.7040 | -747.9 | -205.6 | |
| -1 | -1 | -1 | -1 | -17.74 | 51.81 | -39.18 | 119.89 | 0.6964 | 999999 | 999999 | |
| 11 | -1 | 7 | -1 | -18.18 | 51.43 | -39.57 | 120.24 | 0.7029 | -838.8 | 999999 | |
| 0 | 3 | 0 | 2 | -17.66 | 50.53 | -40.46 | 119.08 | 0.7098 | -312.0 | -250.8 | |
| 3 | 24 | 2 | 17 | -18.35 | 50.28 | -40.71 | 119.83 | 0.7159 | -516.3 | 90.8 | |
| 0 | 4 | 0 | 3 | -16.30 | 50.83 | -40.16 | 117.46 | 0.6999 | -611.0 | -498.5 | |
| 0 | 4 | 0 | 3 | -18.78 | 50.05 | -40.95 | 120.25 | 0.7206 | -289.0 | -145.7 | |
| 0 | 10 | 0 | 7 | -18.97 | 49.71 | -41.28 | 120.30 | 0.7250 | -492.0 | -290.8 | |
| 15 | 55 | 11 | 42 | -21.45 | 46.66 | -44.33 | 121.77 | 0.7673 | -711.4 | -301.0 | |
| 0 | 3 | 0 | 3 | -22.67 | 44.76 | -46.23 | 122.27 | 0.7904 | 480.0 | 579.2 | |
| 5 | 65 | 4 | 50 | -19.56 | 45.70 | -45.30 | 119.03 | 0.7682 | 1090.8 | 692.4 | |
| 0 | 8 | 0 | 6 | -18.75 | 45.62 | -45.37 | 118.01 | 0.7656 | 829.0 | 596.4 | |
| 8 | -12 | 6 | -12 | -19.62 | 45.13 | -45.86 | 118.85 | 0.7740 | 487.5 | 999999 | |
| 0 | 4 | 0 | 4 | -20.31 | 44.13 | -46.86 | 119.22 | 0.7864 | 591.0 | 521.8 | |
| 0 | 2 | 0 | 2 | -20.54 | 43.73 | -47.27 | 119.31 | 0.7911 | 624.0 | 609.1 | |
| 13 | 56 | 11 | 46 | -21.15 | 42.64 | -48.35 | 119.56 | 0.8034 | 755.2 | 526.5 | |
| -17 | -17 | -17 | -17 | -21.04 | 42.24 | -48.75 | 119.26 | 0.8066 | 999999 | 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. | |