SOHO MDI 2002-08-02 03:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74 | 362 | 38 | 186 | -8.31 | 144.91 | -0.72 | 177.55 | 0.2512 | 108.6 | 191.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 9 | 0 | 5 | -8.79 | 150.68 | 5.04 | 198.97 | 0.2684 | -570.0 | -463.0 | |
| 0 | 6 | 0 | 3 | -7.07 | 149.30 | 3.66 | 195.83 | 0.2336 | 851.0 | 598.8 | |
| 2 | 22 | 1 | 11 | -7.10 | 148.54 | 2.91 | 192.64 | 0.2310 | 1202.4 | 982.6 | |
| 7 | 98 | 3 | 50 | -7.83 | 148.30 | 2.67 | 191.03 | 0.2424 | -751.5 | -553.4 | |
| 25 | -4 | 13 | -4 | -7.83 | 147.66 | 2.03 | 188.44 | 0.2405 | -1452.7 | 999999 | |
| 0 | 5 | 0 | 2 | -6.82 | 147.66 | 2.03 | 189.09 | 0.2234 | 455.0 | 396.2 | |
| 0 | 7 | 0 | 4 | -8.28 | 146.91 | 1.28 | 185.15 | 0.2465 | -1013.0 | -759.8 | |
| 0 | 4 | 0 | 2 | -7.83 | 146.47 | 0.83 | 183.49 | 0.2384 | -613.0 | -494.6 | |
| 0 | 3 | 0 | 2 | -8.97 | 145.55 | -0.08 | 179.68 | 0.2573 | -547.0 | -449.9 | |
| 6 | 23 | 3 | 12 | -8.15 | 145.19 | -0.44 | 178.19 | 0.2436 | -798.0 | -480.8 | |
| 2 | -10 | 1 | -10 | -7.87 | 144.99 | -0.64 | 177.32 | 0.2389 | -717.0 | 999999 | |
| 0 | 13 | 0 | 7 | -8.48 | 144.35 | -1.28 | 174.90 | 0.2500 | 906.0 | 635.7 | |
| 0 | 4 | 0 | 2 | -7.42 | 144.35 | -1.28 | 174.50 | 0.2321 | -324.0 | -208.0 | |
| 0 | 4 | 0 | 2 | -7.51 | 143.75 | -1.88 | 172.00 | 0.2347 | 524.0 | 550.7 | |
| 0 | 5 | 0 | 3 | -9.79 | 143.46 | -2.17 | 172.13 | 0.2738 | -593.0 | -442.7 | |
| 0 | 4 | 0 | 2 | -7.63 | 143.43 | -2.20 | 170.75 | 0.2375 | 794.0 | 567.7 | |
| 0 | 13 | 0 | 6 | -8.16 | 143.19 | -2.44 | 170.13 | 0.2471 | 1125.0 | 782.3 | |
| 0 | 6 | 0 | 3 | -8.25 | 142.19 | -3.44 | 166.30 | 0.2520 | 859.0 | 813.4 | |
| 28 | 110 | 15 | 57 | -9.06 | 141.94 | -3.69 | 166.14 | 0.2665 | 1652.9 | 698.2 | |
| 4 | 26 | 2 | 13 | -8.45 | 141.51 | -4.12 | 163.95 | 0.2584 | 1146.5 | 849.5 | |
| 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. | |