SDO HMI 2011-11-13 14:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.78 | 385.86 | 31.75 | 223.19 | 16.20 | 63.91 | 28.66 | 296.98 | 0.5192 | -872.5 | -351.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.72 | 367.54 | 1.00 | 212.92 | 16.43 | 64.51 | 29.25 | 296.91 | 0.5277 | -799.5 | -378.0 | |
| 0.00 | 1.12 | 0.00 | 0.66 | 18.82 | 64.76 | 29.50 | 300.84 | 0.5450 | -794.0 | -655.2 | |
| 52.54 | -1.00 | 30.46 | -1.00 | 16.04 | 64.19 | 28.94 | 296.43 | 0.5214 | -1333.7 | 999999 | |
| 0.52 | 2.49 | 0.29 | 1.41 | 14.09 | 62.28 | 27.02 | 294.08 | 0.4846 | -908.3 | -740.0 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 14.54 | 62.13 | 26.87 | 295.07 | 0.4850 | -605.0 | -437.9 | |
| 0.00 | 1.20 | 0.00 | 0.69 | 17.46 | 62.38 | 27.13 | 300.32 | 0.5060 | -721.0 | -509.5 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 17.90 | 57.95 | 22.69 | 305.31 | 0.4518 | 817.0 | 626.2 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 18.73 | 58.03 | 22.77 | 306.78 | 0.4596 | 698.0 | 580.8 | |
| 0.00 | 1.55 | 0.00 | 0.86 | 17.75 | 57.76 | 22.50 | 305.23 | 0.4482 | 932.0 | 716.9 | |
| 0.00 | 0.95 | 0.00 | 0.53 | 19.68 | 56.88 | 21.62 | 309.85 | 0.4538 | 752.0 | 649.1 | |
| 0.00 | 1.72 | 0.00 | 0.96 | 21.19 | 55.91 | 20.65 | 313.72 | 0.4568 | 782.0 | 651.3 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 22.68 | 54.97 | 19.71 | 317.42 | 0.4619 | 824.0 | 687.0 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 21.53 | 54.43 | 19.17 | 316.29 | 0.4440 | 806.0 | 673.2 | |
| 0.00 | 2.24 | 0.00 | 1.23 | 20.94 | 54.08 | 18.82 | 315.78 | 0.4340 | 859.0 | 624.6 | |
| 0.00 | 1.89 | 0.00 | 1.06 | 25.63 | 52.19 | 16.93 | 325.76 | 0.4686 | -798.0 | -593.1 | |
| 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. | |