| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.54 | 41.89 | 11.83 | 26.62 | -20.27 | 64.98 | -37.40 | 114.54 | 0.6283 | -59.3 | -52.6 | |
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back to the solar disc SDO HMI 2011-02-08 22:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.54 | 2.22 | 0.95 | 1.37 | -20.51 | 67.63 | -34.74 | 116.04 | 0.5963 | 855.8 | 788.0 | |
| 0.00 | 1.11 | 0.00 | 0.69 | -20.95 | 66.85 | -35.52 | 116.38 | 0.6079 | 582.0 | 576.6 | |
| 4.19 | 7.18 | 2.60 | 4.46 | -20.68 | 66.85 | -35.52 | 115.94 | 0.6068 | 819.1 | 519.1 | |
| 0.00 | 0.68 | 0.00 | 0.42 | -19.67 | 67.00 | -35.38 | 114.41 | 0.6009 | 674.0 | 619.5 | |
| 0.43 | 2.31 | 0.26 | 1.43 | -19.47 | 66.70 | -35.67 | 113.96 | 0.6039 | 830.4 | 722.1 | |
| 0.00 | 1.37 | 0.00 | 0.85 | -19.56 | 66.56 | -35.81 | 114.03 | 0.6060 | 665.0 | 544.6 | |
| 0.77 | 2.91 | 0.48 | 1.82 | -20.05 | 66.12 | -36.25 | 114.63 | 0.6134 | 709.6 | 538.7 | |
| 1.28 | 1.45 | 0.81 | 0.92 | -21.09 | 65.56 | -36.82 | 116.00 | 0.6244 | 589.6 | 552.3 | |
| 0.00 | 1.37 | 0.00 | 0.87 | -19.69 | 64.92 | -37.45 | 113.59 | 0.6271 | -757.0 | -558.9 | |
| 0.00 | 3.50 | 0.00 | 2.24 | -20.26 | 64.64 | -37.73 | 114.35 | 0.6325 | -868.0 | -651.0 | |
| 1.28 | 2.91 | 0.82 | 1.86 | -20.59 | 64.51 | -37.87 | 114.80 | 0.6353 | -659.2 | -554.1 | |
| 1.79 | 1.97 | 1.15 | 1.26 | -20.08 | 64.29 | -38.08 | 113.95 | 0.6361 | -810.5 | -738.5 | |
| 0.00 | 0.77 | 0.00 | 0.50 | -19.73 | 63.67 | -38.70 | 113.19 | 0.6426 | -601.0 | -565.6 | |
| 0.00 | 2.31 | 0.00 | 1.49 | -19.75 | 63.46 | -38.91 | 113.14 | 0.6452 | -651.0 | -552.8 | |
| 0.00 | 1.88 | 0.00 | 1.23 | -20.47 | 62.80 | -39.58 | 113.98 | 0.6556 | -813.0 | -704.6 | |
| 3.50 | 3.42 | 2.29 | 2.23 | -20.16 | 62.77 | -39.60 | 113.51 | 0.6550 | -845.2 | 0.0 | |
| 3.76 | 4.53 | 2.47 | 2.98 | -20.38 | 62.45 | -39.92 | 113.74 | 0.6595 | -661.5 | -496.9 | |
| 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. | |