SDO HMI 2011-05-10 00:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.45 | 106.76 | 24.60 | 107.76 | 16.73 | 52.09 | 57.90 | 291.32 | 0.8727 | -450.1 | -255.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.72 | 0.00 | 0.75 | 17.20 | 53.17 | 58.98 | 291.55 | 0.8822 | 136.0 | 153.0 | |
| 0.36 | 83.11 | 0.37 | 84.50 | 16.77 | 52.82 | 58.64 | 291.16 | 0.8787 | -108.0 | -283.5 | |
| 0.00 | 6.27 | 0.00 | 6.47 | 17.28 | 52.78 | 58.59 | 291.74 | 0.8793 | 199.0 | 211.7 | |
| 0.00 | 0.99 | 0.00 | 0.98 | 15.44 | 51.78 | 57.60 | 289.94 | 0.8677 | 178.0 | 72.6 | |
| 20.06 | -2.00 | 20.33 | -2.00 | 16.71 | 52.31 | 58.12 | 291.23 | 0.8745 | -592.0 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.88 | 16.28 | 51.33 | 57.15 | 291.00 | 0.8658 | -455.0 | -496.7 | |
| 0.00 | 0.81 | 0.00 | 0.79 | 15.95 | 51.18 | 57.00 | 290.67 | 0.8639 | -576.0 | -493.9 | |
| 0.00 | 1.25 | 0.00 | 1.23 | 16.56 | 51.17 | 56.98 | 291.36 | 0.8650 | -438.0 | -445.8 | |
| 0.00 | 1.07 | 0.00 | 1.05 | 16.32 | 51.00 | 56.82 | 291.14 | 0.8632 | -536.0 | -488.6 | |
| 0.00 | 1.07 | 0.00 | 1.03 | 16.20 | 50.49 | 56.30 | 291.15 | 0.8587 | -613.0 | -557.7 | |
| 4.03 | 8.24 | 3.90 | 7.95 | 16.75 | 50.56 | 56.38 | 291.75 | 0.8605 | -439.5 | -398.0 | |
| 0.00 | 0.81 | 0.00 | 0.77 | 16.25 | 50.17 | 55.98 | 291.29 | 0.8561 | -660.0 | -614.8 | |
| 0.00 | 1.07 | 0.00 | 0.99 | 18.37 | 48.06 | 53.87 | 294.33 | 0.8434 | -401.0 | -352.2 | |
| 0.00 | 0.45 | 0.00 | 0.37 | 16.65 | 44.50 | 50.32 | 293.53 | 0.8064 | 588.0 | 521.4 | |
| 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. | |