SDO HMI 2011-05-30 18:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.60 | 101.08 | 11.81 | 67.69 | 15.61 | 40.33 | -39.39 | 65.31 | 0.6745 | -251.9 | -207.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 0.57 | 18.75 | 46.36 | -33.35 | 57.36 | 0.6205 | 624.0 | 530.7 | |
| 0.00 | 0.99 | 0.00 | 0.64 | 18.82 | 45.10 | -34.61 | 58.11 | 0.6355 | 695.0 | 584.6 | |
| 0.00 | 0.90 | 0.00 | 0.60 | 16.27 | 41.29 | -38.43 | 63.95 | 0.6664 | -559.0 | -465.8 | |
| 14.89 | 74.65 | 9.85 | 49.32 | 15.38 | 41.13 | -38.59 | 65.29 | 0.6643 | -1039.7 | -375.6 | |
| 0.00 | 4.24 | 0.00 | 2.84 | 15.49 | 40.29 | -39.43 | 65.54 | 0.6746 | -574.0 | -443.1 | |
| 0.00 | 1.99 | 0.00 | 1.34 | 15.14 | 39.83 | -39.88 | 66.24 | 0.6786 | -580.0 | -499.2 | |
| 0.00 | 2.17 | 0.00 | 1.47 | 15.84 | 39.63 | -40.09 | 65.36 | 0.6839 | -483.0 | -308.4 | |
| 0.00 | 1.26 | 0.00 | 0.87 | 15.35 | 38.62 | -41.09 | 66.49 | 0.6935 | 748.0 | 595.1 | |
| 0.00 | 1.53 | 0.00 | 1.09 | 17.08 | 36.75 | -42.96 | 64.95 | 0.7214 | 691.0 | 549.8 | |
| 0.00 | 2.08 | 0.00 | 1.47 | 15.81 | 36.76 | -42.96 | 66.64 | 0.7165 | 688.0 | 501.0 | |
| 0.00 | 1.08 | 0.00 | 0.77 | 15.72 | 36.48 | -43.24 | 66.87 | 0.7193 | 715.0 | 614.8 | |
| 0.00 | 0.54 | 0.00 | 0.39 | 16.13 | 36.19 | -43.52 | 66.44 | 0.7240 | 512.0 | 490.0 | |
| 0.00 | 0.90 | 0.00 | 0.64 | 15.72 | 36.26 | -43.46 | 66.96 | 0.7218 | 618.0 | 565.7 | |
| 2.71 | 7.85 | 1.96 | 5.68 | 16.65 | 35.60 | -44.11 | 65.99 | 0.7323 | 586.3 | 628.0 | |
| 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. | |