SDO HMI 2011-02-11 23:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.77 | 129.23 | 34.76 | 73.01 | -19.64 | 36.02 | -26.31 | 119.58 | 0.4809 | 57.9 | -76.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.67 | 45.60 | 14.11 | 25.08 | -19.33 | 39.33 | -23.00 | 121.71 | 0.4352 | 1034.3 | 401.3 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -18.56 | 39.10 | -23.22 | 119.89 | 0.4330 | 666.0 | 465.9 | |
| 0.43 | 2.40 | 0.24 | 1.33 | -19.29 | 38.38 | -23.95 | 120.73 | 0.4476 | 854.6 | 683.8 | |
| 6.33 | 8.47 | 3.53 | 4.72 | -18.90 | 37.20 | -25.13 | 118.94 | 0.4609 | 862.4 | 604.2 | |
| 2.31 | 3.51 | 1.29 | 1.96 | -18.69 | 36.54 | -25.78 | 117.99 | 0.4686 | 679.0 | 550.6 | |
| 1.20 | 1.45 | 0.67 | 0.82 | -18.33 | 36.18 | -26.14 | 117.02 | 0.4715 | -615.1 | -595.3 | |
| 0.00 | 1.20 | 0.00 | 0.68 | -19.51 | 35.45 | -26.87 | 118.78 | 0.4880 | -725.0 | -552.4 | |
| 0.00 | 1.28 | 0.00 | 0.73 | -19.59 | 35.16 | -27.17 | 118.70 | 0.4924 | -759.0 | -626.5 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -19.18 | 34.95 | -27.37 | 117.78 | 0.4929 | -920.0 | -771.0 | |
| 0.00 | 1.63 | 0.00 | 0.93 | -19.71 | 34.46 | -27.86 | 118.42 | 0.5023 | -787.0 | -579.4 | |
| 0.00 | 0.86 | 0.00 | 0.49 | -20.61 | 34.25 | -28.07 | 119.93 | 0.5104 | 731.0 | 665.4 | |
| 15.40 | 29.18 | 8.80 | 16.66 | -19.22 | 34.45 | -27.88 | 117.50 | 0.4998 | -1006.8 | -639.2 | |
| 2.48 | -12.00 | 1.42 | -12.00 | -18.88 | 34.40 | -27.92 | 116.84 | 0.4986 | -1021.9 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.69 | -20.57 | 34.08 | -28.25 | 119.74 | 0.5123 | 994.0 | 772.5 | |
| 0.00 | 2.31 | 0.00 | 1.32 | -19.54 | 34.24 | -28.08 | 117.97 | 0.5043 | -647.0 | -539.7 | |
| 1.88 | 3.08 | 1.09 | 1.78 | -20.71 | 33.73 | -28.60 | 119.73 | 0.5177 | 841.5 | 684.1 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -20.46 | 33.60 | -28.73 | 119.19 | 0.5179 | 788.0 | 498.3 | |
| 0.34 | 4.45 | 0.20 | 2.55 | -19.03 | 33.74 | -28.59 | 116.68 | 0.5083 | -794.8 | -635.9 | |
| 0.00 | 1.37 | 0.00 | 0.79 | -19.25 | 33.37 | -28.95 | 116.85 | 0.5143 | -666.0 | -429.6 | |
| 0.00 | 1.63 | 0.00 | 0.95 | -20.48 | 32.94 | -29.38 | 118.79 | 0.5266 | 777.0 | 557.7 | |
| 0.00 | 0.94 | 0.00 | 0.55 | -21.25 | 32.45 | -29.88 | 119.81 | 0.5372 | -630.0 | -518.2 | |
| 0.00 | 1.03 | 0.00 | 0.61 | -21.87 | 31.86 | -30.46 | 120.48 | 0.5481 | 616.0 | 478.9 | |
| 0.00 | 1.20 | 0.00 | 0.71 | -22.43 | 31.46 | -30.86 | 121.16 | 0.5562 | -473.0 | -512.3 | |
| 4.28 | 5.82 | 2.54 | 3.46 | -21.89 | 31.26 | -31.06 | 120.13 | 0.5558 | -1007.0 | -721.8 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -20.92 | 31.49 | -30.83 | 118.63 | 0.5476 | -794.0 | -697.2 | |
| 1.45 | 4.45 | 0.87 | 2.65 | -22.13 | 31.09 | -31.23 | 120.42 | 0.5592 | -760.6 | -661.9 | |
| 0.00 | 1.63 | 0.00 | 0.97 | -21.63 | 31.03 | -31.30 | 119.55 | 0.5573 | -713.0 | -543.3 | |
| 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. | |