| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.63 | 40.46 | 12.12 | 43.06 | 16.81 | 178.22 | -58.09 | 66.69 | 0.8864 | 23.5 | 71.1 | |
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back to the solar disc SDO HMI 2011-02-26 02:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.81 | 2.50 | 1.85 | 2.56 | 17.27 | 179.59 | -56.72 | 65.73 | 0.8777 | -372.7 | -364.5 | |
| 0.00 | 1.64 | 0.00 | 1.74 | 18.70 | 178.87 | -57.45 | 64.44 | 0.8869 | -92.0 | -172.7 | |
| 3.53 | 11.28 | 3.55 | 11.36 | 15.48 | 179.67 | -56.65 | 67.65 | 0.8724 | 705.8 | 571.0 | |
| 2.41 | 3.10 | 2.46 | 3.16 | 16.08 | 179.35 | -56.97 | 67.10 | 0.8765 | 369.1 | 346.5 | |
| 0.00 | 1.03 | 0.00 | 1.14 | 18.95 | 177.84 | -58.47 | 64.53 | 0.8949 | -453.0 | -365.1 | |
| 0.00 | 1.72 | 0.00 | 1.76 | 15.65 | 179.25 | -57.06 | 67.60 | 0.8761 | 383.0 | 324.1 | |
| 0.00 | 1.29 | 0.00 | 1.37 | 17.07 | 178.47 | -57.84 | 66.32 | 0.8856 | -238.0 | -252.0 | |
| 2.76 | 4.65 | 2.97 | 5.00 | 17.38 | 178.02 | -58.29 | 66.14 | 0.8896 | -510.8 | -409.3 | |
| 0.00 | 2.15 | 0.00 | 2.34 | 17.26 | 177.67 | -58.65 | 66.39 | 0.8919 | -293.0 | -246.2 | |
| 1.12 | 3.70 | 1.29 | 4.26 | 18.81 | 176.44 | -59.88 | 65.14 | 0.9042 | -321.9 | -317.2 | |
| 0.00 | 1.98 | 0.00 | 2.10 | 15.88 | 177.98 | -58.33 | 67.77 | 0.8863 | 576.0 | 553.9 | |
| 0.00 | 1.03 | 0.00 | 1.12 | 16.01 | 177.45 | -58.87 | 67.81 | 0.8905 | 338.0 | 296.1 | |
| 0.00 | 0.60 | 0.00 | 0.70 | 17.56 | 175.58 | -60.74 | 66.74 | 0.9071 | -248.0 | -209.0 | |
| 0.00 | 3.79 | 0.00 | 4.45 | 17.24 | 175.24 | -61.07 | 67.17 | 0.9087 | -268.0 | -168.1 | |
| 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. | |