| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.73 | 41.85 | 8.49 | 27.61 | -20.19 | 64.40 | -40.18 | 113.42 | 0.6619 | -173.7 | -78.2 | |
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back to the solar disc SDO HMI 2011-02-08 18:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.45 | 3.67 | 0.92 | 2.33 | -20.63 | 67.22 | -37.36 | 115.10 | 0.6294 | 764.8 | 679.0 | |
| 0.00 | 1.54 | 0.00 | 0.98 | -19.80 | 66.74 | -37.84 | 113.64 | 0.6323 | 885.0 | 665.7 | |
| 0.00 | 0.85 | 0.00 | 0.55 | -19.79 | 66.58 | -38.00 | 113.56 | 0.6342 | 622.0 | 514.9 | |
| 0.00 | 2.65 | 0.00 | 1.69 | -19.51 | 66.54 | -38.04 | 113.12 | 0.6338 | 900.0 | 716.5 | |
| 0.00 | 2.56 | 0.00 | 1.65 | -20.54 | 66.25 | -38.33 | 114.57 | 0.6409 | 695.0 | 551.0 | |
| 0.00 | 1.03 | 0.00 | 0.66 | -19.56 | 66.29 | -38.29 | 113.09 | 0.6371 | 583.0 | 491.2 | |
| 0.00 | 1.28 | 0.00 | 0.83 | -20.09 | 66.05 | -38.52 | 113.82 | 0.6417 | 355.0 | 316.3 | |
| 1.79 | 2.56 | 1.16 | 1.66 | -20.96 | 65.71 | -38.87 | 115.00 | 0.6489 | 654.3 | 513.6 | |
| 0.00 | 1.11 | 0.00 | 0.73 | -20.50 | 64.75 | -39.83 | 113.96 | 0.6588 | -613.0 | -629.1 | |
| 0.00 | 0.85 | 0.00 | 0.56 | -20.22 | 64.83 | -39.74 | 113.58 | 0.6570 | -757.0 | -648.8 | |
| 0.00 | 1.11 | 0.00 | 0.73 | -19.72 | 64.66 | -39.92 | 112.78 | 0.6575 | -665.0 | -512.5 | |
| 0.00 | 0.85 | 0.00 | 0.56 | -20.14 | 64.53 | -40.05 | 113.36 | 0.6604 | -719.0 | -608.9 | |
| 0.00 | 1.03 | 0.00 | 0.68 | -19.68 | 63.64 | -40.94 | 112.39 | 0.6697 | -867.0 | -681.2 | |
| 0.00 | 2.65 | 0.00 | 1.77 | -19.70 | 63.46 | -41.11 | 112.36 | 0.6718 | -698.0 | -565.2 | |
| 0.00 | 1.11 | 0.00 | 0.74 | -19.81 | 63.26 | -41.32 | 112.46 | 0.6745 | -404.0 | -404.5 | |
| 5.13 | 17.00 | 3.46 | 11.49 | -20.18 | 62.85 | -41.73 | 112.87 | 0.6804 | -777.7 | -600.2 | |
| 4.36 | -16.00 | 2.95 | -16.00 | -20.40 | 62.56 | -42.02 | 113.10 | 0.6844 | -617.3 | 999999 | |
| 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. | |