SDO HMI 2011-05-03 00:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.75 | 188.24 | 39.97 | 130.29 | 16.74 | 47.23 | -39.49 | 60.86 | 0.6993 | -150.0 | -98.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.78 | 16.33 | 49.27 | -37.46 | 60.22 | 0.6747 | -732.0 | -621.3 | |
| 0.00 | 0.54 | 0.00 | 0.36 | 16.73 | 49.05 | -37.67 | 59.82 | 0.6792 | -302.0 | -300.3 | |
| 0.00 | 0.71 | 0.00 | 0.48 | 15.70 | 49.01 | -37.71 | 61.23 | 0.6741 | -686.0 | -592.1 | |
| 7.59 | 111.31 | 5.11 | 75.86 | 16.33 | 48.75 | -37.97 | 60.55 | 0.6804 | -871.3 | -344.2 | |
| 3.12 | -4.00 | 2.11 | -4.00 | 16.62 | 48.68 | -38.04 | 60.20 | 0.6828 | -834.7 | 999999 | |
| 1.07 | 4.11 | 0.72 | 2.77 | 16.01 | 48.62 | -38.10 | 61.05 | 0.6801 | -561.4 | -502.1 | |
| 1.07 | 2.23 | 0.72 | 1.50 | 15.59 | 48.63 | -38.09 | 61.60 | 0.6778 | -647.0 | -557.1 | |
| 24.10 | -4.00 | 16.47 | -4.00 | 17.06 | 48.17 | -38.55 | 59.92 | 0.6908 | -913.3 | 999999 | |
| 0.00 | 1.16 | 0.00 | 0.80 | 17.69 | 47.89 | -38.83 | 59.27 | 0.6973 | -374.0 | -313.1 | |
| 0.00 | 2.50 | 0.00 | 1.76 | 19.16 | 47.12 | -39.60 | 57.86 | 0.7135 | -542.0 | -479.7 | |
| 0.00 | 3.03 | 0.00 | 2.11 | 17.84 | 47.44 | -39.28 | 59.35 | 0.7029 | -691.0 | -427.0 | |
| 0.00 | 0.62 | 0.00 | 0.43 | 16.17 | 47.86 | -38.86 | 61.28 | 0.6895 | -87.0 | -140.4 | |
| 0.00 | 1.16 | 0.00 | 0.80 | 17.58 | 47.39 | -39.34 | 59.71 | 0.7021 | 184.0 | 129.8 | |
| 0.00 | 0.80 | 0.00 | 0.55 | 16.15 | 47.70 | -39.02 | 61.40 | 0.6911 | -484.0 | -384.0 | |
| 0.00 | 0.62 | 0.00 | 0.43 | 16.49 | 47.33 | -39.39 | 61.16 | 0.6969 | 231.0 | 158.3 | |
| 0.80 | 2.59 | 0.55 | 1.78 | 16.20 | 47.28 | -39.44 | 61.57 | 0.6960 | 280.0 | 167.2 | |
| 1.43 | -16.00 | 0.98 | -16.00 | 16.10 | 47.26 | -39.46 | 61.71 | 0.6957 | -382.5 | 999999 | |
| 0.00 | 2.05 | 0.00 | 1.42 | 16.02 | 47.00 | -39.73 | 61.96 | 0.6983 | -388.0 | -289.9 | |
| 0.00 | 0.80 | 0.00 | 0.56 | 16.31 | 46.26 | -40.46 | 61.98 | 0.7077 | 524.0 | 550.1 | |
| 1.79 | 3.30 | 1.22 | 2.26 | 14.28 | 46.70 | -40.02 | 64.44 | 0.6932 | 772.5 | 627.4 | |
| 0.00 | 1.52 | 0.00 | 1.04 | 14.06 | 46.66 | -40.06 | 64.75 | 0.6925 | 803.0 | 742.7 | |
| 0.00 | 1.34 | 0.00 | 0.93 | 15.16 | 46.34 | -40.38 | 63.46 | 0.7013 | 573.0 | 443.6 | |
| 0.00 | 1.34 | 0.00 | 0.92 | 14.19 | 46.51 | -40.21 | 64.65 | 0.6949 | 489.0 | 418.5 | |
| 0.00 | 0.80 | 0.00 | 0.56 | 15.10 | 46.10 | -40.62 | 63.65 | 0.7037 | 574.0 | 543.0 | |
| 0.98 | 1.61 | 0.69 | 1.13 | 16.28 | 45.65 | -41.07 | 62.36 | 0.7143 | 699.5 | 646.4 | |
| 0.00 | 1.07 | 0.00 | 0.78 | 19.13 | 44.84 | -41.89 | 59.18 | 0.7368 | 514.0 | 415.2 | |
| 2.41 | 3.30 | 1.75 | 2.40 | 18.84 | 44.88 | -41.84 | 59.52 | 0.7348 | 700.8 | 586.9 | |
| 0.80 | 4.91 | 0.56 | 3.43 | 14.99 | 45.75 | -40.97 | 63.98 | 0.7071 | 765.2 | 635.3 | |
| 0.00 | 0.27 | 0.00 | 0.19 | 16.85 | 45.08 | -41.65 | 61.92 | 0.7231 | 609.0 | 574.3 | |
| 4.11 | 6.78 | 2.92 | 4.82 | 16.20 | 45.21 | -41.52 | 62.69 | 0.7187 | 678.6 | 540.5 | |
| 3.84 | 6.16 | 2.78 | 4.45 | 16.85 | 44.35 | -42.37 | 62.29 | 0.7309 | 763.3 | 475.8 | |
| 0.00 | 1.25 | 0.00 | 0.92 | 18.43 | 43.84 | -42.88 | 60.57 | 0.7435 | 544.0 | 485.9 | |
| 0.00 | 3.12 | 0.00 | 2.26 | 16.47 | 44.28 | -42.44 | 62.81 | 0.7298 | 710.0 | 618.6 | |
| 0.00 | 1.16 | 0.00 | 0.85 | 17.10 | 44.02 | -42.70 | 62.15 | 0.7354 | 584.0 | 512.8 | |
| 0.00 | 1.79 | 0.00 | 1.30 | 16.49 | 43.98 | -42.74 | 62.94 | 0.7331 | 665.0 | 590.9 | |
| 4.64 | 10.27 | 3.39 | 7.51 | 16.82 | 43.71 | -43.01 | 62.65 | 0.7374 | 709.8 | 534.6 | |
| 0.00 | 2.86 | 0.00 | 2.15 | 18.43 | 42.70 | -44.02 | 61.16 | 0.7550 | 593.0 | 483.8 | |
| 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. | |