SDO HMI 2011-02-10 03:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.44 | 34.31 | 4.36 | 20.27 | 19.48 | 65.91 | -20.56 | 37.30 | 0.5472 | -61.0 | -99.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.63 | 3.25 | 0.95 | 1.89 | 19.33 | 68.13 | -18.34 | 34.53 | 0.5260 | -829.8 | -770.9 | |
| 2.22 | 9.15 | 1.29 | 5.33 | 19.15 | 67.72 | -18.75 | 35.32 | 0.5273 | -992.3 | -812.7 | |
| 0.00 | 0.43 | 0.00 | 0.25 | 19.36 | 67.36 | -19.11 | 35.59 | 0.5329 | -688.0 | -581.0 | |
| 0.00 | 1.37 | 0.00 | 0.79 | 18.41 | 67.41 | -19.06 | 36.64 | 0.5213 | -147.0 | -137.8 | |
| 0.00 | 1.97 | 0.00 | 1.15 | 19.50 | 67.08 | -19.39 | 35.82 | 0.5370 | -768.0 | -706.3 | |
| 2.82 | 4.96 | 1.66 | 2.92 | 19.71 | 66.95 | -19.52 | 35.76 | 0.5404 | -718.1 | -606.9 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 19.29 | 66.64 | -19.83 | 36.67 | 0.5383 | -602.0 | -543.7 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 19.40 | 66.52 | -19.94 | 36.70 | 0.5405 | -539.0 | -447.4 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 20.90 | 64.56 | -21.91 | 37.53 | 0.5745 | 503.0 | 482.8 | |
| 0.00 | 1.88 | 0.00 | 1.13 | 20.64 | 64.53 | -21.94 | 37.87 | 0.5719 | 685.0 | 663.5 | |
| 0.77 | 2.48 | 0.46 | 1.50 | 19.68 | 63.14 | -23.33 | 40.69 | 0.5742 | 1026.1 | 761.2 | |
| 0.00 | 1.20 | 0.00 | 0.72 | 19.50 | 62.82 | -23.65 | 41.28 | 0.5753 | 846.0 | 765.2 | |
| 0.00 | 4.88 | 0.00 | 2.95 | 19.32 | 62.51 | -23.96 | 41.87 | 0.5764 | 946.0 | 724.8 | |
| 0.00 | 0.34 | 0.00 | 0.22 | 21.11 | 59.29 | -27.18 | 43.26 | 0.6242 | 589.0 | 590.5 | |
| 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. | |