SDO HMI 2011-10-12 11:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.00 | 31.87 | 3.61 | 16.55 | 20.03 | 109.45 | 10.55 | 324.83 | 0.2994 | 376.1 | 399.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.61 | 21.19 | 115.58 | 16.68 | 314.71 | 0.3782 | 743.0 | 639.1 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 22.37 | 113.17 | 14.27 | 321.22 | 0.3655 | 809.0 | 621.4 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 19.97 | 112.21 | 13.31 | 318.31 | 0.3269 | -604.0 | -492.8 | |
| 0.00 | 1.14 | 0.00 | 0.60 | 20.13 | 112.00 | 13.10 | 319.09 | 0.3264 | -866.0 | -647.0 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 20.11 | 111.54 | 12.64 | 320.02 | 0.3212 | -846.0 | -678.5 | |
| 0.00 | 2.63 | 0.00 | 1.37 | 20.60 | 110.40 | 11.50 | 323.57 | 0.3157 | -995.0 | -783.8 | |
| 0.00 | 0.61 | 0.00 | 0.32 | 19.87 | 109.93 | 11.03 | 323.19 | 0.3016 | 678.0 | 578.6 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 19.48 | 109.54 | 10.64 | 323.29 | 0.2927 | 726.0 | 567.4 | |
| 0.00 | 1.58 | 0.00 | 0.84 | 25.66 | 109.60 | 10.70 | 333.59 | 0.3779 | 837.0 | 704.6 | |
| 0.00 | 0.79 | 0.00 | 0.41 | 19.30 | 109.05 | 10.15 | 324.18 | 0.2855 | 691.0 | 564.6 | |
| 0.00 | 0.70 | 0.00 | 0.36 | 19.43 | 108.83 | 9.93 | 325.03 | 0.2851 | 688.0 | 583.8 | |
| 3.41 | 19.95 | 1.76 | 10.30 | 19.25 | 108.50 | 9.60 | 325.54 | 0.2795 | 963.8 | 769.1 | |
| 3.59 | -12.00 | 1.85 | -12.00 | 19.53 | 108.39 | 9.49 | 326.43 | 0.2822 | 1047.0 | 999999 | |
| 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. | |