SDO HMI 2011-08-11 21:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.78 | 0.00 | 8.03 | 16.72 | 222.67 | 30.58 | 291.35 | 0.5264 | -387.0 | -370.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.72 | 0.00 | 0.44 | 19.45 | 226.66 | 34.58 | 294.47 | 0.5901 | -701.0 | -544.9 | |
| 0.00 | 0.81 | 0.00 | 0.49 | 19.85 | 225.12 | 33.04 | 295.88 | 0.5722 | -623.0 | -543.7 | |
| 0.00 | 1.17 | 0.00 | 0.71 | 19.51 | 225.01 | 32.92 | 295.37 | 0.5691 | -753.0 | -615.2 | |
| 0.00 | 1.08 | 0.00 | 0.66 | 22.09 | 225.22 | 33.14 | 299.49 | 0.5841 | -681.0 | -513.2 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 18.68 | 224.32 | 32.24 | 294.29 | 0.5566 | -721.0 | -580.9 | |
| 0.00 | 1.44 | 0.00 | 0.85 | 18.15 | 223.65 | 31.57 | 293.72 | 0.5454 | -625.0 | -536.5 | |
| 0.00 | 2.53 | 0.00 | 1.44 | 14.04 | 221.26 | 29.18 | 287.14 | 0.4969 | -844.0 | -725.3 | |
| 0.00 | 0.54 | 0.00 | 0.31 | 13.80 | 221.23 | 29.14 | 286.67 | 0.4957 | -643.0 | -596.3 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 13.93 | 221.07 | 28.98 | 287.00 | 0.4938 | -908.0 | -711.6 | |
| 0.00 | 0.90 | 0.00 | 0.51 | 13.69 | 221.00 | 28.91 | 286.54 | 0.4920 | -753.0 | -586.9 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 18.00 | 220.77 | 28.69 | 295.03 | 0.5059 | 666.0 | 536.3 | |
| 0.00 | 1.53 | 0.00 | 0.86 | 14.20 | 220.07 | 27.99 | 287.96 | 0.4802 | 904.0 | 729.4 | |
| 0.00 | 0.54 | 0.00 | 0.30 | 13.42 | 219.65 | 27.57 | 286.54 | 0.4715 | 651.0 | 565.5 | |
| 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. | |