SDO HMI 2011-05-27 07:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 73.87 | 130.81 | 39.61 | 70.19 | 20.63 | 130.57 | 5.10 | 347.65 | 0.3849 | -53.5 | -177.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.98 | 0.00 | 1.07 | 20.77 | 133.06 | 7.59 | 341.78 | 0.3966 | -488.0 | -213.5 | |
| 24.72 | 64.15 | 13.35 | 34.62 | 21.07 | 132.58 | 7.11 | 343.09 | 0.3987 | -1098.0 | -413.4 | |
| 5.86 | -2.00 | 3.16 | -2.00 | 20.84 | 132.15 | 6.67 | 343.90 | 0.3932 | -1083.3 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 20.31 | 131.47 | 6.00 | 345.08 | 0.3821 | -902.0 | -746.7 | |
| 0.90 | 5.95 | 0.49 | 3.21 | 21.26 | 130.95 | 5.48 | 346.92 | 0.3949 | -826.3 | -654.7 | |
| 1.71 | -5.00 | 0.92 | -5.00 | 21.46 | 130.83 | 5.36 | 347.32 | 0.3976 | -880.5 | 999999 | |
| 0.45 | 1.71 | 0.24 | 0.92 | 21.42 | 130.50 | 5.03 | 348.06 | 0.3959 | -595.8 | -445.1 | |
| 1.62 | 1.89 | 0.87 | 1.01 | 19.95 | 130.13 | 4.65 | 348.10 | 0.3714 | 663.0 | 684.3 | |
| 4.60 | 13.71 | 2.46 | 7.33 | 20.63 | 128.98 | 3.50 | 351.28 | 0.3789 | 900.0 | 605.2 | |
| 1.53 | 2.80 | 0.81 | 1.48 | 19.46 | 128.76 | 3.28 | 351.32 | 0.3595 | 1030.9 | 863.8 | |
| 2.89 | -9.00 | 1.54 | -9.00 | 20.44 | 128.71 | 3.24 | 351.85 | 0.3751 | 764.7 | 999999 | |
| 29.59 | 35.73 | 15.77 | 19.04 | 20.21 | 127.93 | 2.46 | 353.73 | 0.3698 | 1012.3 | 674.1 | |
| 0.00 | 2.08 | 0.00 | 1.07 | 15.38 | 126.07 | 0.59 | 358.00 | 0.2879 | -902.0 | -736.0 | |
| 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. | |