SDO HMI 2011-06-03 06:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.84 | 36.82 | 6.30 | 19.38 | 17.23 | 41.27 | 7.88 | 337.73 | 0.3363 | -6.8 | 38.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.86 | 13.93 | 4.74 | 7.44 | 18.14 | 45.44 | 12.04 | 328.07 | 0.3766 | -1025.4 | -849.3 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 21.51 | 45.20 | 11.81 | 332.99 | 0.4210 | 725.0 | 589.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 16.12 | 42.89 | 9.50 | 330.91 | 0.3274 | -939.0 | -702.1 | |
| 2.62 | 3.07 | 1.37 | 1.61 | 16.88 | 41.51 | 8.12 | 335.57 | 0.3282 | -908.9 | -760.2 | |
| 0.00 | 1.63 | 0.00 | 0.85 | 16.31 | 41.01 | 7.61 | 336.17 | 0.3162 | -781.0 | -697.5 | |
| 0.00 | 3.07 | 0.00 | 1.59 | 15.07 | 40.01 | 6.62 | 337.40 | 0.2908 | -688.0 | -566.4 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 16.72 | 37.32 | 3.93 | 347.46 | 0.3034 | 899.0 | 620.2 | |
| 0.36 | 1.99 | 0.19 | 1.03 | 16.46 | 37.16 | 3.76 | 347.78 | 0.2987 | 968.2 | 811.6 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.43 | 36.87 | 3.48 | 348.66 | 0.2972 | 912.0 | 734.4 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.24 | 36.14 | 2.74 | 350.90 | 0.2919 | 965.0 | 719.0 | |
| 0.00 | 1.81 | 0.00 | 0.94 | 16.62 | 35.89 | 2.50 | 351.90 | 0.2975 | 819.0 | 678.8 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 16.27 | 35.66 | 2.27 | 352.47 | 0.2912 | 1057.0 | 829.9 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 16.59 | 35.60 | 2.21 | 352.81 | 0.2964 | 889.0 | 731.0 | |
| 0.00 | 1.90 | 0.00 | 0.99 | 17.39 | 35.13 | 1.74 | 354.59 | 0.3087 | 970.0 | 702.4 | |
| 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. | |