SDO HMI 2011-02-12 17:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.36 | 177.46 | 36.57 | 94.78 | -20.30 | 34.92 | -17.54 | 130.68 | 0.3725 | -107.8 | 124.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.37 | 0.00 | 0.71 | -19.34 | 39.88 | -12.58 | 137.15 | 0.3035 | 416.0 | 331.8 | |
| 4.54 | 34.14 | 2.35 | 17.73 | -18.79 | 39.60 | -12.86 | 135.21 | 0.3004 | 1300.1 | 870.6 | |
| 1.37 | -2.00 | 0.71 | -2.00 | -19.09 | 39.52 | -12.95 | 135.76 | 0.3048 | 1021.1 | 999999 | |
| 1.97 | -2.00 | 1.02 | -2.00 | -18.97 | 39.36 | -13.10 | 135.14 | 0.3052 | 1026.4 | 999999 | |
| 7.87 | 9.67 | 4.10 | 5.04 | -18.88 | 38.54 | -13.93 | 133.26 | 0.3141 | 972.9 | 702.8 | |
| 1.88 | 2.74 | 0.98 | 1.43 | -19.02 | 38.07 | -14.39 | 132.71 | 0.3212 | 773.1 | 597.2 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -19.38 | 35.76 | -16.70 | 129.58 | 0.3533 | -145.0 | -128.8 | |
| 0.00 | 2.82 | 0.00 | 1.50 | -19.98 | 35.66 | -16.80 | 130.80 | 0.3604 | 446.0 | 424.6 | |
| 0.00 | 2.99 | 0.00 | 1.60 | -21.28 | 35.05 | -17.41 | 132.63 | 0.3806 | 777.0 | 882.8 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -20.84 | 34.87 | -17.59 | 131.45 | 0.3785 | 938.0 | 727.6 | |
| 0.00 | 7.27 | 0.00 | 3.89 | -20.56 | 34.84 | -17.63 | 130.81 | 0.3762 | 671.0 | 769.4 | |
| 2.65 | 4.45 | 1.43 | 2.39 | -21.78 | 34.65 | -17.81 | 133.06 | 0.3904 | 828.9 | 812.4 | |
| 1.54 | 42.10 | 0.82 | 22.39 | -19.05 | 34.98 | -17.49 | 127.63 | 0.3602 | -897.3 | -832.9 | |
| 0.77 | 1.71 | 0.41 | 0.92 | -21.54 | 34.58 | -17.88 | 132.46 | 0.3888 | 1091.3 | 931.8 | |
| 0.00 | 1.71 | 0.00 | 0.92 | -21.02 | 34.62 | -17.85 | 131.44 | 0.3833 | 960.0 | 703.5 | |
| 5.82 | -13.00 | 3.09 | -13.00 | -18.80 | 34.84 | -17.62 | 126.86 | 0.3598 | -1188.5 | 999999 | |
| 0.00 | 3.34 | 0.00 | 1.78 | -20.01 | 34.70 | -17.76 | 129.41 | 0.3726 | -594.0 | -573.1 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -21.32 | 34.44 | -18.02 | 131.81 | 0.3883 | 814.0 | 675.1 | |
| 0.00 | 4.02 | 0.00 | 2.17 | -21.77 | 34.28 | -18.18 | 132.50 | 0.3946 | 827.0 | 513.8 | |
| 1.45 | 3.85 | 0.78 | 2.06 | -20.63 | 34.20 | -18.27 | 130.02 | 0.3847 | 864.6 | 678.8 | |
| 0.00 | 0.51 | 0.00 | 0.27 | -19.93 | 34.22 | -18.25 | 128.54 | 0.3780 | -722.0 | -561.3 | |
| 17.46 | -13.00 | 9.30 | -13.00 | -19.05 | 34.25 | -18.21 | 126.62 | 0.3696 | -998.5 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.60 | -21.84 | 33.70 | -18.76 | 131.81 | 0.4022 | 764.0 | 554.8 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -18.56 | 34.05 | -18.42 | 125.19 | 0.3681 | -599.0 | -474.1 | |
| 0.00 | 2.74 | 0.00 | 1.48 | -22.12 | 33.60 | -18.86 | 132.21 | 0.4061 | 438.0 | 313.9 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -20.65 | 33.76 | -18.70 | 129.45 | 0.3902 | 846.0 | 626.4 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -20.46 | 33.72 | -18.74 | 129.00 | 0.3891 | 622.0 | 537.9 | |
| 0.00 | 1.37 | 0.00 | 0.74 | -21.58 | 33.27 | -19.19 | 130.69 | 0.4049 | 679.0 | 554.1 | |
| 0.00 | 1.54 | 0.00 | 0.83 | -20.87 | 33.10 | -19.37 | 129.01 | 0.4005 | 789.0 | 552.1 | |
| 0.00 | 2.82 | 0.00 | 1.55 | -23.27 | 32.20 | -20.26 | 132.53 | 0.4335 | -710.0 | -644.5 | |
| 2.05 | 3.68 | 1.12 | 2.01 | -22.09 | 32.18 | -20.28 | 130.27 | 0.4228 | -943.5 | -814.5 | |
| 1.37 | 4.79 | 0.75 | 2.63 | -22.92 | 32.02 | -20.45 | 131.65 | 0.4324 | -959.2 | -796.1 | |
| 6.67 | 7.36 | 3.66 | 4.04 | -21.87 | 31.22 | -21.24 | 128.67 | 0.4324 | -1099.7 | -832.8 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -21.50 | 31.14 | -21.32 | 127.85 | 0.4302 | -934.0 | -830.2 | |
| 10.95 | 22.68 | 6.05 | 12.51 | -22.47 | 30.75 | -21.71 | 129.26 | 0.4434 | -986.1 | -691.0 | |
| 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. | |