SDO HMI 2011-11-10 03:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79.55 | 162.31 | 45.00 | 91.90 | -25.10 | 85.19 | 4.36 | 188.12 | 0.4856 | -175.1 | -47.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.22 | 60.94 | 13.84 | 34.85 | -25.74 | 87.60 | 6.78 | 192.31 | 0.5008 | 1083.9 | 336.4 | |
| 0.00 | 1.47 | 0.00 | 0.83 | -25.09 | 87.30 | 6.48 | 192.08 | 0.4903 | 987.0 | 782.8 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -24.72 | 87.19 | 6.36 | 192.04 | 0.4844 | 858.0 | 630.1 | |
| 6.55 | 7.67 | 3.68 | 4.30 | -24.07 | 86.24 | 5.41 | 190.56 | 0.4718 | 953.9 | 760.5 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -26.27 | 85.31 | 4.48 | 188.04 | 0.5026 | 510.0 | 313.9 | |
| 0.00 | 2.93 | 0.00 | 1.64 | -23.80 | 84.44 | 3.61 | 187.17 | 0.4633 | -707.0 | -569.1 | |
| 18.79 | 36.89 | 10.50 | 20.64 | -24.00 | 83.85 | 3.03 | 185.98 | 0.4653 | -1056.1 | -313.5 | |
| 1.72 | 45.77 | 0.98 | 25.89 | -25.41 | 83.46 | 2.63 | 184.92 | 0.4864 | -832.0 | -654.8 | |
| 0.00 | 3.62 | 0.00 | 2.04 | -24.77 | 83.25 | 2.42 | 184.64 | 0.4763 | -486.0 | -408.4 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -25.95 | 83.21 | 2.38 | 184.35 | 0.4944 | -518.0 | -426.9 | |
| 16.03 | -8.00 | 9.07 | -8.00 | -25.38 | 83.10 | 2.27 | 184.25 | 0.4855 | -1057.1 | 999999 | |
| 2.59 | -8.00 | 1.46 | -8.00 | -24.87 | 82.93 | 2.10 | 184.01 | 0.4775 | -1028.2 | 999999 | |
| 9.65 | -8.00 | 5.47 | -8.00 | -25.48 | 82.61 | 1.78 | 183.32 | 0.4865 | -930.4 | 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. | |