SOHO MDI 2002-08-01 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64 | 295 | 33 | 150 | -8.44 | 144.92 | -3.36 | 167.72 | 0.2598 | 419.6 | 128.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | -8.74 | 150.56 | 2.28 | 188.86 | 0.2562 | -879.0 | -762.4 | |
| 0 | 4 | 0 | 2 | -8.41 | 150.03 | 1.76 | 187.01 | 0.2495 | -712.0 | -494.2 | |
| 0 | 3 | 0 | 1 | -8.82 | 150.04 | 1.76 | 186.82 | 0.2564 | -539.0 | -423.7 | |
| 0 | 3 | 0 | 1 | -9.31 | 150.00 | 1.72 | 186.46 | 0.2645 | -818.0 | -725.1 | |
| 0 | 4 | 0 | 2 | -7.39 | 148.95 | 0.67 | 182.91 | 0.2306 | 900.0 | 821.5 | |
| 3 | 24 | 2 | 12 | -7.27 | 148.51 | 0.24 | 181.03 | 0.2282 | 1304.7 | 994.8 | |
| 10 | 98 | 5 | 50 | -7.84 | 147.76 | -0.52 | 177.82 | 0.2381 | -911.2 | -805.1 | |
| 12 | -7 | 6 | -7 | -7.96 | 147.16 | -1.12 | 175.36 | 0.2408 | -1575.6 | 999999 | |
| 5 | -7 | 2 | -7 | -8.17 | 146.80 | -1.48 | 173.97 | 0.2448 | -1348.7 | 999999 | |
| 0 | 9 | 0 | 4 | -8.50 | 146.52 | -1.76 | 173.00 | 0.2509 | -1024.0 | -819.6 | |
| 0 | 5 | 0 | 3 | -8.74 | 146.23 | -2.04 | 172.04 | 0.2556 | -665.0 | -564.9 | |
| 0 | 4 | 0 | 2 | -7.93 | 145.92 | -2.36 | 170.29 | 0.2428 | -619.0 | -511.2 | |
| 0 | 4 | 0 | 2 | -8.01 | 144.84 | -3.44 | 166.08 | 0.2480 | -433.0 | -527.6 | |
| 0 | 3 | 0 | 2 | -8.23 | 143.24 | -5.04 | 160.30 | 0.2593 | 829.0 | 775.0 | |
| 0 | 3 | 0 | 1 | -8.40 | 142.39 | -5.89 | 157.56 | 0.2671 | 801.0 | 668.6 | |
| 0 | 5 | 0 | 3 | -10.70 | 142.15 | -6.13 | 159.75 | 0.3046 | 534.0 | 463.7 | |
| 31 | 109 | 16 | 56 | -9.14 | 142.06 | -6.22 | 157.49 | 0.2808 | 1688.4 | 907.7 | |
| 3 | -17 | 2 | -17 | -8.49 | 141.74 | -6.53 | 155.52 | 0.2728 | 1194.2 | 999999 | |
| 0 | 6 | 0 | 3 | -7.54 | 139.75 | -8.53 | 147.48 | 0.2748 | 493.0 | 434.9 | |
| 0 | 5 | 0 | 3 | -8.73 | 135.16 | -13.12 | 138.01 | 0.3369 | 709.0 | 538.6 | |
| 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. | |