SOHO MDI 2000-07-07 03:11:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40 | 254 | 25 | 156 | -19.99 | 17.02 | -28.08 | 131.76 | 0.5937 | -530.7 | -109.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6 | 99 | 4 | 59 | -19.30 | 20.08 | -25.02 | 133.88 | 0.5559 | -1095.6 | -717.1 | |
| 12 | -1 | 7 | -1 | -18.84 | 19.92 | -25.17 | 133.06 | 0.5531 | -1494.2 | 999999 | |
| 0 | 5 | 0 | 3 | -19.19 | 18.04 | -27.06 | 131.57 | 0.5764 | 113.0 | 276.1 | |
| 9 | 18 | 5 | 11 | -19.47 | 17.52 | -27.58 | 131.43 | 0.5844 | -1142.3 | -799.7 | |
| 0 | 3 | 0 | 2 | -22.01 | 16.57 | -28.53 | 133.85 | 0.6162 | 881.0 | 667.2 | |
| 0 | 4 | 0 | 2 | -19.44 | 17.05 | -28.05 | 130.93 | 0.5891 | -870.0 | -587.9 | |
| 3 | 12 | 2 | 7 | -20.05 | 16.74 | -28.36 | 131.46 | 0.5976 | -613.9 | -501.6 | |
| 0 | 23 | 0 | 14 | -19.61 | 15.76 | -29.33 | 129.96 | 0.6042 | -320.0 | -112.8 | |
| 0 | 3 | 0 | 2 | -20.48 | 15.59 | -29.51 | 130.95 | 0.6132 | -207.0 | -117.4 | |
| 0 | 3 | 0 | 2 | -21.09 | 15.26 | -29.84 | 131.46 | 0.6217 | 485.0 | 478.6 | |
| 4 | 35 | 3 | 22 | -21.81 | 14.85 | -30.25 | 132.01 | 0.6317 | 1374.4 | 880.4 | |
| 0 | 5 | 0 | 3 | -19.54 | 15.25 | -29.85 | 129.40 | 0.6092 | -338.0 | -372.0 | |
| 3 | -11 | 2 | -11 | -22.17 | 14.56 | -30.53 | 132.21 | 0.6375 | 563.4 | 999999 | |
| 0 | 3 | 0 | 2 | -21.48 | 14.28 | -30.82 | 131.09 | 0.6348 | 467.0 | 373.2 | |
| 0 | 3 | 0 | 2 | -20.87 | 14.17 | -30.92 | 130.22 | 0.6311 | 709.0 | 638.8 | |
| 0 | 14 | 0 | 9 | -20.44 | 14.17 | -30.92 | 129.65 | 0.6277 | 1006.0 | 749.2 | |
| 0 | 4 | 0 | 3 | -21.07 | 13.33 | -31.77 | 129.77 | 0.6414 | 735.0 | 546.6 | |
| 0 | 13 | 0 | 8 | -20.86 | 13.08 | -32.02 | 129.29 | 0.6424 | 834.0 | 751.6 | |
| 3 | 7 | 2 | 5 | -20.79 | 12.70 | -32.40 | 128.88 | 0.6458 | 644.9 | 539.3 | |
| 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. | |