SDO HMI 2011-11-15 22:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.41 | 102.08 | 141.77 | 406.61 | 19.63 | 87.92 | 83.44 | 289.47 | 0.9915 | -112.7 | -75.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.96 | 28.36 | 44.91 | 201.22 | 19.06 | 90.89 | 86.41 | 288.91 | 0.9975 | -254.6 | -63.1 | |
| 3.44 | -1.00 | 25.82 | -1.00 | 19.22 | 91.37 | 86.90 | 289.09 | 0.9980 | 323.6 | 999999 | |
| 0.00 | 1.46 | 0.00 | 4.71 | 18.35 | 86.01 | 81.53 | 288.14 | 0.9886 | 69.0 | 0.9 | |
| 0.00 | 1.72 | 0.00 | 6.49 | 19.22 | 87.54 | 83.07 | 289.02 | 0.9921 | -551.0 | -447.5 | |
| 1.89 | 13.40 | 6.25 | 42.67 | 18.93 | 86.27 | 81.80 | 288.73 | 0.9893 | 333.1 | -338.1 | |
| 4.90 | -5.00 | 15.40 | -5.00 | 18.83 | 85.81 | 81.33 | 288.62 | 0.9881 | -320.8 | 999999 | |
| 0.00 | 1.20 | 0.00 | 4.37 | 19.45 | 87.18 | 82.70 | 289.26 | 0.9913 | -257.0 | -257.1 | |
| 0.00 | 11.86 | 0.00 | 32.53 | 19.86 | 84.49 | 80.01 | 289.69 | 0.9846 | -294.0 | -149.6 | |
| 0.00 | 1.12 | 0.00 | 2.73 | 19.55 | 83.02 | 78.54 | 289.39 | 0.9800 | 250.0 | 296.9 | |
| 1.89 | 42.96 | 4.70 | 111.89 | 20.27 | 83.19 | 78.72 | 290.12 | 0.9807 | 436.3 | 56.6 | |
| 12.55 | -10.00 | 35.14 | -10.00 | 20.97 | 84.63 | 80.15 | 290.80 | 0.9850 | -423.0 | 999999 | |
| 0.86 | -10.00 | 2.50 | -10.00 | 21.39 | 85.04 | 80.57 | 291.23 | 0.9862 | 160.8 | 999999 | |
| 2.92 | -10.00 | 7.05 | -10.00 | 20.60 | 82.84 | 78.37 | 290.47 | 0.9795 | 366.5 | 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. | |