| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.14 | 55.74 | 14.71 | 33.99 | -19.56 | 35.80 | -34.23 | 114.63 | 0.5848 | -53.0 | 19.4 | |
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back to the solar disc SDO HMI 2011-02-11 09:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.56 | -22.03 | 39.85 | -30.18 | 121.00 | 0.5458 | -668.0 | -481.1 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -20.72 | 39.52 | -30.51 | 118.54 | 0.5426 | 782.0 | 603.7 | |
| 1.97 | 2.91 | 1.16 | 1.72 | -19.41 | 38.60 | -31.43 | 115.74 | 0.5482 | 885.2 | 788.7 | |
| 1.97 | 5.74 | 1.17 | 3.40 | -19.37 | 38.38 | -31.64 | 115.55 | 0.5507 | 739.1 | 648.5 | |
| 0.00 | 0.94 | 0.00 | 0.56 | -19.28 | 37.96 | -32.07 | 115.17 | 0.5559 | 593.0 | 435.5 | |
| 3.94 | 7.62 | 2.34 | 4.53 | -19.01 | 37.91 | -32.12 | 114.67 | 0.5554 | 840.6 | 563.5 | |
| 3.00 | 3.68 | 1.79 | 2.20 | -19.16 | 37.39 | -32.64 | 114.67 | 0.5628 | 438.1 | 194.8 | |
| 0.00 | 1.20 | 0.00 | 0.72 | -18.67 | 37.43 | -32.60 | 113.86 | 0.5603 | 667.0 | 502.4 | |
| 0.00 | 2.23 | 0.00 | 1.36 | -19.28 | 35.37 | -34.66 | 113.92 | 0.5896 | 118.0 | 190.9 | |
| 5.22 | 9.76 | 3.21 | 6.00 | -19.69 | 35.04 | -34.99 | 114.44 | 0.5954 | -837.8 | -448.0 | |
| 0.00 | 1.11 | 0.00 | 0.69 | -19.14 | 34.63 | -35.40 | 113.38 | 0.5984 | -762.0 | -582.2 | |
| 0.00 | 1.63 | 0.00 | 1.01 | -19.70 | 34.34 | -35.69 | 114.16 | 0.6043 | -687.0 | -637.3 | |
| 0.00 | 1.37 | 0.00 | 0.85 | -19.87 | 34.14 | -35.89 | 114.35 | 0.6075 | -561.0 | -462.8 | |
| 6.93 | 10.53 | 4.31 | 6.54 | -19.01 | 34.01 | -36.02 | 112.92 | 0.6059 | -853.7 | -656.0 | |
| 0.00 | 1.54 | 0.00 | 0.97 | -20.82 | 33.21 | -36.82 | 115.45 | 0.6227 | 803.0 | 624.2 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -20.95 | 32.77 | -37.26 | 115.46 | 0.6285 | 628.0 | 488.5 | |
| 1.11 | 2.48 | 0.73 | 1.63 | -22.03 | 30.56 | -39.47 | 116.20 | 0.6590 | -680.5 | -628.4 | |
| 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. | |