SOHO MDI 2000-07-04 09:35:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33 | 202 | 26 | 162 | 19.09 | 30.75 | -50.53 | 68.16 | 0.7876 | 461.2 | -13.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10 | 42 | 8 | 32 | 19.62 | 34.14 | -47.14 | 66.65 | 0.7544 | 991.5 | 402.4 | |
| 4 | -1 | 3 | -1 | 19.81 | 33.75 | -47.53 | 66.51 | 0.7590 | 823.7 | 999999 | |
| 0 | 3 | 0 | 2 | 18.69 | 33.81 | -47.48 | 67.94 | 0.7556 | -563.0 | -454.4 | |
| 0 | 13 | 0 | 10 | 20.07 | 32.95 | -48.33 | 66.41 | 0.7679 | 706.0 | 503.5 | |
| 0 | 5 | 0 | 4 | 20.97 | 31.46 | -49.82 | 65.68 | 0.7852 | 309.0 | 311.2 | |
| 0 | 17 | 0 | 13 | 18.72 | 32.35 | -48.93 | 68.29 | 0.7709 | -288.0 | -290.5 | |
| 0 | 5 | 0 | 4 | 20.38 | 31.33 | -49.95 | 66.45 | 0.7850 | 496.0 | 356.1 | |
| 0 | 7 | 0 | 5 | 19.64 | 30.60 | -50.69 | 67.56 | 0.7906 | -342.0 | -331.6 | |
| 8 | 33 | 6 | 27 | 18.63 | 30.43 | -50.86 | 68.85 | 0.7903 | -755.7 | -599.2 | |
| 0 | 5 | 0 | 4 | 18.96 | 29.48 | -51.81 | 68.65 | 0.8003 | 377.0 | 265.2 | |
| 0 | 1 | 0 | 1 | 18.67 | 29.33 | -51.95 | 69.04 | 0.8011 | -120.0 | -94.5 | |
| 11 | 49 | 9 | 42 | 19.00 | 28.43 | -52.86 | 68.82 | 0.8105 | 838.6 | 174.8 | |
| 0 | 8 | 0 | 6 | 18.23 | 28.77 | -52.52 | 69.70 | 0.8058 | -862.0 | -667.7 | |
| 0 | 6 | 0 | 5 | 18.12 | 28.26 | -53.02 | 69.93 | 0.8106 | -245.0 | -282.2 | |
| 0 | 5 | 0 | 4 | 17.68 | 27.68 | -53.60 | 70.57 | 0.8154 | -446.0 | -412.7 | |
| 0 | 3 | 0 | 3 | 17.28 | 27.79 | -53.50 | 71.05 | 0.8138 | -614.0 | -507.6 | |
| 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. | |