| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 44.88 | 201.83 | 24.73 | 111.31 | 9.19 | 357.43 | -24.38 | 67.70 | 0.4421 | -707.3 | -362.7 | |
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back to the solar disc SDO HMI 2011-12-11 22:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.11 | 181.71 | 0.61 | 99.98 | 9.77 | 357.83 | -23.98 | 66.17 | 0.4396 | -667.1 | -435.0 | |
| 33.89 | -1.00 | 18.65 | -1.00 | 9.30 | 357.80 | -24.01 | 67.22 | 0.4373 | -1361.9 | 999999 | |
| 3.41 | -1.00 | 1.88 | -1.00 | 8.94 | 357.46 | -24.34 | 68.25 | 0.4402 | -1014.0 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.89 | 8.10 | 357.32 | -24.48 | 70.16 | 0.4380 | -841.0 | -621.1 | |
| 2.38 | -1.00 | 1.32 | -1.00 | 9.03 | 357.16 | -24.64 | 68.29 | 0.4451 | -740.5 | 999999 | |
| 2.30 | 4.09 | 1.27 | 2.27 | 8.88 | 356.71 | -25.09 | 68.94 | 0.4509 | -840.5 | -757.7 | |
| 1.28 | 1.70 | 0.71 | 0.94 | 8.61 | 356.66 | -25.14 | 69.54 | 0.4502 | -747.8 | -758.4 | |
| 0.00 | 1.28 | 0.00 | 0.71 | 9.03 | 356.47 | -25.34 | 68.80 | 0.4552 | -476.0 | -392.3 | |
| 0.00 | 0.43 | 0.00 | 0.24 | 8.59 | 355.14 | -26.67 | 70.60 | 0.4724 | -441.0 | -510.6 | |
| 0.51 | 3.07 | 0.29 | 1.73 | 8.41 | 354.65 | -27.15 | 71.26 | 0.4787 | 960.0 | 777.6 | |
| 0.00 | 1.53 | 0.00 | 0.87 | 8.41 | 354.35 | -27.46 | 71.44 | 0.4832 | 1001.0 | 828.1 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 8.11 | 354.03 | -27.77 | 72.21 | 0.4865 | 778.0 | 681.8 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 8.62 | 353.62 | -28.18 | 71.44 | 0.4946 | 830.0 | 694.8 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 9.19 | 353.20 | -28.61 | 70.59 | 0.5032 | 776.0 | 651.4 | |
| 0.00 | 0.85 | 0.00 | 0.49 | 8.87 | 352.71 | -29.09 | 71.48 | 0.5087 | 780.0 | 617.8 | |
| 0.00 | 1.62 | 0.00 | 0.94 | 7.41 | 350.77 | -31.04 | 75.14 | 0.5311 | 791.0 | 660.2 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 8.37 | 350.20 | -31.61 | 73.65 | 0.5426 | 581.0 | 531.3 | |
| 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. | |