SDO HMI 2011-08-10 04:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.63 | 87.24 | 23.73 | 49.84 | 19.85 | 241.86 | 27.18 | 300.07 | 0.4974 | 256.5 | 141.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.06 | 5.24 | 2.46 | 3.17 | 19.13 | 248.30 | 33.62 | 294.50 | 0.5771 | -774.1 | -621.5 | |
| 0.00 | 4.34 | 0.00 | 2.60 | 18.89 | 247.63 | 32.95 | 294.41 | 0.5673 | -730.0 | -689.7 | |
| 0.00 | 3.61 | 0.00 | 2.16 | 18.43 | 247.34 | 32.66 | 293.78 | 0.5616 | -810.0 | -712.7 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 20.81 | 247.00 | 32.32 | 297.97 | 0.5681 | -625.0 | -463.5 | |
| 0.00 | 0.72 | 0.00 | 0.42 | 18.75 | 245.55 | 30.88 | 295.26 | 0.5394 | -519.0 | -402.5 | |
| 9.21 | 14.72 | 5.40 | 8.63 | 18.41 | 245.45 | 30.77 | 294.72 | 0.5365 | -842.7 | -677.3 | |
| 2.53 | 3.43 | 1.46 | 1.98 | 18.13 | 243.84 | 29.16 | 295.12 | 0.5135 | -897.2 | -687.4 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 20.06 | 240.84 | 26.17 | 300.84 | 0.4844 | 829.0 | 659.8 | |
| 0.00 | 2.80 | 0.00 | 1.59 | 20.72 | 240.89 | 26.22 | 302.03 | 0.4893 | 849.0 | 652.3 | |
| 0.00 | 1.17 | 0.00 | 0.66 | 21.80 | 240.05 | 25.37 | 304.75 | 0.4861 | 941.0 | 742.6 | |
| 0.00 | 2.26 | 0.00 | 1.27 | 21.55 | 239.28 | 24.60 | 305.01 | 0.4746 | 845.0 | 561.4 | |
| 1.63 | 3.61 | 0.91 | 2.02 | 20.39 | 239.04 | 24.36 | 303.05 | 0.4632 | 682.2 | 626.1 | |
| 0.00 | 1.72 | 0.00 | 0.98 | 23.67 | 239.61 | 24.94 | 308.47 | 0.4951 | 688.0 | 467.9 | |
| 9.21 | 23.57 | 5.12 | 13.11 | 19.87 | 238.81 | 24.13 | 302.24 | 0.4565 | 1087.0 | 647.9 | |
| 3.16 | -14.00 | 1.76 | -14.00 | 20.16 | 238.71 | 24.04 | 302.89 | 0.4573 | 954.8 | 999999 | |
| 9.75 | 12.74 | 5.46 | 7.13 | 21.13 | 238.84 | 24.17 | 304.63 | 0.4660 | 913.4 | 709.0 | |
| 2.08 | 4.43 | 1.16 | 2.46 | 20.86 | 238.37 | 23.69 | 304.60 | 0.4580 | 1027.0 | 853.6 | |
| 0.00 | 0.72 | 0.00 | 0.40 | 22.34 | 237.06 | 22.38 | 308.77 | 0.4535 | 902.0 | 711.2 | |
| 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. | |