| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.48 | 26.22 | 3.22 | 15.08 | -20.31 | 70.16 | 28.11 | 240.48 | 0.5087 | 235.9 | 98.1 | |
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back to the solar disc SDO HMI 2011-02-13 12:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.94 | 2.06 | 0.55 | 1.21 | -20.03 | 72.83 | 30.78 | 242.96 | 0.5420 | 635.8 | 726.7 | |
| 1.54 | 1.80 | 0.91 | 1.06 | -20.31 | 72.75 | 30.70 | 242.43 | 0.5423 | 661.2 | 547.0 | |
| 3.00 | 3.94 | 1.76 | 2.31 | -20.11 | 72.48 | 30.43 | 242.61 | 0.5379 | 889.6 | 766.5 | |
| 0.00 | 1.37 | 0.00 | 0.80 | -19.45 | 72.16 | 30.11 | 243.58 | 0.5304 | 722.0 | 621.7 | |
| 0.00 | 1.20 | 0.00 | 0.70 | -20.07 | 72.04 | 29.99 | 242.41 | 0.5319 | 767.0 | 739.3 | |
| 0.00 | 2.14 | 0.00 | 1.26 | -21.84 | 72.25 | 30.20 | 239.47 | 0.5442 | 672.0 | 494.1 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -19.13 | 71.38 | 29.33 | 243.69 | 0.5183 | 811.0 | 675.6 | |
| 0.00 | 2.31 | 0.00 | 1.35 | -21.34 | 71.80 | 29.75 | 240.03 | 0.5357 | 737.0 | 507.2 | |
| 0.00 | 1.63 | 0.00 | 0.95 | -21.16 | 71.25 | 29.20 | 239.98 | 0.5276 | 761.0 | 578.1 | |
| 0.00 | 3.94 | 0.00 | 2.22 | -19.16 | 68.44 | 26.39 | 241.63 | 0.4791 | -888.0 | -664.4 | |
| 0.00 | 2.23 | 0.00 | 1.23 | -20.49 | 64.78 | 22.73 | 235.76 | 0.4397 | -738.0 | -574.2 | |
| 0.00 | 0.77 | 0.00 | 0.42 | -19.99 | 64.33 | 22.28 | 236.30 | 0.4300 | -552.0 | -474.4 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -20.71 | 63.35 | 21.30 | 233.77 | 0.4230 | -734.0 | -593.4 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -20.99 | 62.44 | 20.39 | 232.12 | 0.4139 | -721.0 | -609.5 | |
| 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. | |