SDO HMI 2014-08-11 21:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.09 | 0.00 | 13.16 | 11.54 | 173.71 | 46.97 | 279.96 | 0.7252 | 38.5 | 31.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.82 | 13.60 | 180.36 | 53.62 | 282.17 | 0.8027 | -394.0 | -372.2 | |
| 0.00 | 0.99 | 0.00 | 0.81 | 11.89 | 179.78 | 53.04 | 280.04 | 0.7963 | -233.0 | -272.8 | |
| 0.00 | 1.26 | 0.00 | 1.01 | 9.55 | 179.14 | 52.40 | 277.08 | 0.7895 | -224.0 | -273.4 | |
| 0.00 | 0.81 | 0.00 | 0.66 | 11.59 | 179.65 | 52.91 | 279.67 | 0.7949 | -354.0 | -375.8 | |
| 0.00 | 1.89 | 0.00 | 1.53 | 13.56 | 179.41 | 52.66 | 282.17 | 0.7929 | -445.0 | -337.4 | |
| 0.00 | 1.35 | 0.00 | 1.01 | 11.04 | 175.75 | 49.01 | 279.03 | 0.7524 | 517.0 | 474.9 | |
| 0.00 | 0.90 | 0.00 | 0.68 | 11.20 | 175.74 | 49.00 | 279.24 | 0.7523 | 182.0 | 205.1 | |
| 0.00 | 0.99 | 0.00 | 0.73 | 11.02 | 174.85 | 48.11 | 279.04 | 0.7422 | 209.0 | 257.1 | |
| 0.00 | 1.17 | 0.00 | 0.85 | 10.17 | 174.03 | 47.29 | 277.89 | 0.7324 | 310.0 | 343.1 | |
| 0.00 | 1.89 | 0.00 | 1.37 | 9.39 | 173.79 | 47.05 | 276.83 | 0.7296 | 650.0 | 456.1 | |
| 0.00 | 1.26 | 0.00 | 0.88 | 12.89 | 171.56 | 44.82 | 281.82 | 0.7043 | 287.0 | 268.8 | |
| 0.00 | 0.63 | 0.00 | 0.41 | 7.16 | 167.20 | 40.46 | 273.45 | 0.6473 | 616.0 | 465.1 | |
| 0.00 | 1.17 | 0.00 | 0.71 | 11.59 | 161.83 | 35.09 | 281.00 | 0.5759 | -744.0 | -527.5 | |
| 0.00 | 1.71 | 0.00 | 1.04 | 13.92 | 162.02 | 35.28 | 284.96 | 0.5824 | 888.0 | 576.6 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 11.90 | 161.35 | 34.61 | 281.61 | 0.5695 | -688.0 | -607.6 | |
| 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. | |