| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 77.03 | 156.46 | 41.61 | 84.65 | 20.72 | 130.73 | 8.55 | 339.85 | 0.4020 | 27.2 | -63.5 | |
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back to the solar disc SDO HMI 2011-05-27 13:59:10 UT
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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 | 1.08 | 20.61 | 134.47 | 12.29 | 331.81 | 0.4236 | 717.0 | 488.6 | |
| 27.24 | 67.01 | 14.86 | 36.58 | 21.09 | 133.01 | 10.83 | 335.21 | 0.4200 | -1099.2 | -410.2 | |
| 1.26 | 1.53 | 0.69 | 0.83 | 20.79 | 132.33 | 10.15 | 336.28 | 0.4113 | -864.6 | -843.0 | |
| 9.02 | 12.72 | 4.90 | 6.91 | 21.25 | 131.47 | 9.29 | 338.52 | 0.4126 | -971.9 | -813.8 | |
| 2.89 | 5.86 | 1.56 | 3.17 | 20.63 | 131.33 | 9.15 | 338.21 | 0.4027 | -876.4 | -722.5 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 21.38 | 130.42 | 8.24 | 340.85 | 0.4087 | -721.0 | -603.1 | |
| 0.00 | 2.34 | 0.00 | 1.26 | 20.00 | 129.99 | 7.81 | 340.59 | 0.3857 | 554.0 | 478.7 | |
| 0.00 | 2.53 | 0.00 | 1.36 | 20.39 | 129.91 | 7.73 | 341.12 | 0.3912 | 871.0 | 710.4 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 19.54 | 129.54 | 7.36 | 341.20 | 0.3764 | 901.0 | 793.2 | |
| 0.00 | 1.53 | 0.00 | 0.82 | 19.61 | 129.38 | 7.20 | 341.64 | 0.3765 | 871.0 | 741.7 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 21.24 | 129.07 | 6.89 | 343.71 | 0.4001 | -469.0 | -369.0 | |
| 0.00 | 2.07 | 0.00 | 1.11 | 19.48 | 128.83 | 6.65 | 342.86 | 0.3718 | 937.0 | 779.4 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 19.38 | 128.56 | 6.38 | 343.42 | 0.3690 | 830.0 | 700.8 | |
| 9.38 | 18.13 | 5.03 | 9.72 | 20.45 | 128.21 | 6.04 | 345.08 | 0.3842 | 1001.2 | 381.5 | |
| 13.98 | 36.71 | 7.49 | 19.63 | 20.48 | 127.56 | 5.38 | 346.64 | 0.3821 | 946.9 | 668.5 | |
| 13.26 | -15.00 | 7.08 | -15.00 | 19.96 | 127.48 | 5.30 | 346.50 | 0.3736 | 1103.9 | 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 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. | |