| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.73 | 55.98 | 11.87 | 32.00 | -15.62 | 114.31 | -26.58 | 119.94 | 0.4992 | 206.9 | 152.0 | |
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back to the solar disc SDO HMI 2011-05-26 03:59:10 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.26 | 0.00 | 0.71 | -15.26 | 116.32 | -24.58 | 121.03 | 0.4702 | 966.0 | 754.7 | |
| 0.00 | 2.53 | 0.00 | 1.42 | -15.51 | 116.18 | -24.71 | 121.38 | 0.4738 | 805.0 | 665.0 | |
| 6.58 | 12.08 | 3.71 | 6.82 | -16.10 | 116.00 | -24.90 | 122.31 | 0.4805 | 928.4 | 717.3 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -16.51 | 115.81 | -25.09 | 122.86 | 0.4860 | 741.0 | 607.8 | |
| 1.44 | -3.00 | 0.81 | -3.00 | -15.82 | 115.80 | -25.10 | 121.59 | 0.4811 | 748.1 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.77 | -16.31 | 114.99 | -25.91 | 121.75 | 0.4951 | 656.0 | 468.5 | |
| 0.00 | 2.25 | 0.00 | 1.28 | -14.78 | 114.99 | -25.91 | 118.93 | 0.4847 | 776.0 | 632.7 | |
| 0.00 | 1.80 | 0.00 | 1.02 | -14.96 | 114.82 | -26.07 | 119.13 | 0.4881 | 486.0 | 388.6 | |
| 0.00 | 1.80 | 0.00 | 1.03 | -16.37 | 114.59 | -26.30 | 121.50 | 0.5006 | 458.0 | 321.1 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -14.65 | 114.76 | -26.14 | 118.50 | 0.4869 | 734.0 | 509.6 | |
| 0.00 | 2.98 | 0.00 | 1.70 | -14.71 | 114.12 | -26.78 | 118.08 | 0.4958 | 711.0 | 525.6 | |
| 0.36 | 2.16 | 0.21 | 1.24 | -14.76 | 113.83 | -27.07 | 117.95 | 0.5001 | 675.0 | 517.2 | |
| 0.00 | 1.17 | 0.00 | 0.67 | -14.58 | 113.79 | -27.11 | 117.57 | 0.4996 | 712.0 | 623.5 | |
| 0.00 | 0.81 | 0.00 | 0.47 | -15.58 | 113.50 | -27.39 | 119.16 | 0.5095 | -614.0 | -473.8 | |
| 2.25 | 8.30 | 1.29 | 4.76 | -15.29 | 113.51 | -27.39 | 118.66 | 0.5077 | -897.3 | -663.2 | |
| 5.32 | 8.75 | 3.09 | 5.08 | -16.16 | 112.81 | -28.09 | 119.65 | 0.5224 | -852.2 | -585.1 | |
| 4.78 | 6.58 | 2.76 | 3.81 | -15.57 | 112.83 | -28.07 | 118.62 | 0.5184 | -930.5 | -777.0 | |
| 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. | |