SDO HMI 2011-09-06 10:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.04 | 34.45 | 10.31 | 27.04 | -19.43 | 258.51 | 43.90 | 237.56 | 0.7770 | 355.9 | 212.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.16 | 0.00 | 0.92 | -19.01 | 259.48 | 44.87 | 238.58 | 0.7839 | 485.0 | 457.9 | |
| 12.59 | 14.82 | 9.96 | 11.73 | -19.40 | 259.02 | 44.42 | 237.88 | 0.7817 | 649.0 | 462.2 | |
| 0.00 | 3.93 | 0.00 | 3.12 | -20.12 | 258.87 | 44.27 | 236.98 | 0.7839 | 478.0 | 398.6 | |
| 0.45 | 2.05 | 0.35 | 1.62 | -19.63 | 258.61 | 44.00 | 237.39 | 0.7790 | 735.4 | 604.5 | |
| 0.00 | 2.59 | 0.00 | 2.02 | -19.17 | 258.36 | 43.76 | 237.78 | 0.7744 | 750.0 | 623.1 | |
| 0.00 | 0.98 | 0.00 | 0.80 | -21.57 | 259.10 | 44.49 | 235.48 | 0.7932 | 419.0 | 339.8 | |
| 0.00 | 1.16 | 0.00 | 0.91 | -19.53 | 258.26 | 43.66 | 237.31 | 0.7753 | 301.0 | 268.3 | |
| 0.00 | 1.07 | 0.00 | 0.84 | -19.93 | 258.18 | 43.57 | 236.81 | 0.7765 | 551.0 | 380.1 | |
| 0.00 | 0.98 | 0.00 | 0.75 | -18.63 | 257.13 | 42.53 | 237.71 | 0.7600 | -350.0 | -357.7 | |
| 0.00 | 1.96 | 0.00 | 1.50 | -19.07 | 257.23 | 42.62 | 237.25 | 0.7632 | -377.0 | -366.9 | |
| 0.00 | 1.34 | 0.00 | 1.01 | -18.52 | 257.01 | 42.40 | 237.77 | 0.7582 | -736.0 | -587.7 | |
| 0.00 | 0.63 | 0.00 | 0.50 | -22.02 | 258.14 | 43.53 | 234.43 | 0.7872 | 370.0 | 398.3 | |
| 0.00 | 0.89 | 0.00 | 0.65 | -15.60 | 256.03 | 41.42 | 240.69 | 0.7331 | -533.0 | -462.9 | |
| 0.00 | 0.89 | 0.00 | 0.67 | -19.26 | 255.99 | 41.38 | 236.29 | 0.7526 | -519.0 | -399.6 | |
| 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. | |