SOHO MDI 2010-07-11 17:35:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32 | 298 | 25 | 234 | 21.44 | 332.33 | -49.58 | 65.47 | 0.7796 | -177.0 | 117.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | 18.69 | 344.62 | -37.29 | 64.96 | 0.6357 | -633.0 | -517.2 | |
| 0 | 9 | 0 | 6 | 16.69 | 341.77 | -40.14 | 69.05 | 0.6635 | -287.0 | -517.9 | |
| 0 | 3 | 0 | 2 | 16.65 | 340.86 | -41.06 | 69.41 | 0.6745 | -181.0 | -212.8 | |
| 0 | 4 | 0 | 3 | 17.01 | 340.65 | -41.26 | 68.96 | 0.6780 | -445.0 | -459.6 | |
| 0 | 5 | 0 | 3 | 15.35 | 340.85 | -41.06 | 71.31 | 0.6710 | -533.0 | -408.2 | |
| 0 | 2 | 0 | 1 | 16.91 | 340.29 | -41.62 | 69.22 | 0.6821 | -362.0 | -83.4 | |
| 0 | 2 | 0 | 1 | 20.40 | 339.10 | -42.81 | 64.73 | 0.7067 | -400.0 | -340.5 | |
| 0 | 2 | 0 | 1 | 19.53 | 335.44 | -46.48 | 67.08 | 0.7443 | 501.0 | 484.5 | |
| 0 | 9 | 0 | 7 | 20.83 | 333.98 | -47.93 | 65.80 | 0.7630 | 556.0 | 511.8 | |
| 20 | 141 | 15 | 109 | 21.34 | 333.25 | -48.66 | 65.36 | 0.7717 | -800.9 | 31.3 | |
| 0 | 3 | 0 | 3 | 22.56 | 331.61 | -50.30 | 64.28 | 0.7909 | -265.0 | -319.7 | |
| 0 | 4 | 0 | 4 | 22.33 | 331.32 | -50.59 | 64.63 | 0.7932 | -421.0 | -200.1 | |
| 4 | 34 | 3 | 27 | 21.50 | 331.53 | -50.39 | 65.61 | 0.7892 | -380.7 | -159.6 | |
| 0 | 3 | 0 | 2 | 21.13 | 330.76 | -51.15 | 66.26 | 0.7958 | -96.0 | -87.1 | |
| 0 | 2 | 0 | 2 | 24.58 | 328.81 | -53.11 | 62.56 | 0.8216 | 406.0 | 379.0 | |
| 0 | 2 | 0 | 1 | 23.60 | 328.74 | -53.17 | 63.75 | 0.8200 | 575.0 | 485.1 | |
| 0 | 4 | 0 | 3 | 21.56 | 329.44 | -52.47 | 66.04 | 0.8094 | 494.0 | 472.8 | |
| 4 | 64 | 4 | 55 | 22.73 | 328.45 | -53.47 | 64.85 | 0.8209 | 1041.2 | 565.9 | |
| 0 | 2 | 0 | 2 | 23.76 | 327.84 | -54.08 | 63.77 | 0.8284 | 465.0 | 384.5 | |
| 4 | -18 | 3 | -18 | 22.98 | 328.23 | -53.68 | 64.61 | 0.8233 | 786.7 | 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 umbra + penumbra 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 umbra + penumbra 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. | |