SDO HMI 2011-06-11 18:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.47 | 82.59 | 11.51 | 51.77 | -15.60 | 246.41 | -34.49 | 117.00 | 0.6133 | 180.0 | 130.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 5.52 | 0.00 | 3.35 | -15.53 | 249.32 | -31.58 | 118.68 | 0.5772 | 962.0 | 795.3 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -15.79 | 249.02 | -31.88 | 118.87 | 0.5825 | 528.0 | 389.5 | |
| 5.70 | 28.43 | 3.47 | 17.27 | -15.57 | 248.91 | -31.99 | 118.45 | 0.5826 | 847.9 | 701.0 | |
| 6.97 | -3.00 | 4.24 | -3.00 | -15.28 | 248.88 | -32.02 | 117.98 | 0.5813 | 907.2 | 999999 | |
| 0.00 | 3.08 | 0.00 | 1.88 | -15.19 | 248.49 | -32.41 | 117.57 | 0.5857 | 561.0 | 451.8 | |
| 0.00 | 1.54 | 0.00 | 0.94 | -15.51 | 248.36 | -32.54 | 117.98 | 0.5891 | 563.0 | 411.1 | |
| 0.00 | 1.00 | 0.00 | 0.60 | -12.61 | 248.75 | -32.15 | 113.56 | 0.5688 | 479.0 | 381.6 | |
| 0.00 | 1.63 | 0.00 | 1.00 | -15.22 | 248.11 | -32.79 | 117.38 | 0.5907 | 765.0 | 487.7 | |
| 0.00 | 1.99 | 0.00 | 1.23 | -15.26 | 247.69 | -33.21 | 117.17 | 0.5962 | 527.0 | 403.3 | |
| 0.00 | 2.08 | 0.00 | 1.28 | -14.82 | 247.50 | -33.40 | 116.36 | 0.5961 | 491.0 | 479.3 | |
| 0.00 | 1.18 | 0.00 | 0.73 | -14.72 | 247.25 | -33.65 | 116.07 | 0.5988 | 727.0 | 511.9 | |
| 0.00 | 3.89 | 0.00 | 2.41 | -14.76 | 247.02 | -33.88 | 115.98 | 0.6019 | 538.0 | 516.6 | |
| 0.00 | 1.00 | 0.00 | 0.65 | -18.92 | 244.97 | -35.93 | 120.87 | 0.6490 | 618.0 | 390.9 | |
| 0.00 | 1.18 | 0.00 | 0.75 | -16.42 | 244.92 | -35.98 | 117.26 | 0.6362 | -504.0 | -444.8 | |
| 1.36 | 1.99 | 0.87 | 1.28 | -15.22 | 244.18 | -36.72 | 115.09 | 0.6393 | 661.7 | 500.6 | |
| 0.00 | 1.90 | 0.00 | 1.24 | -16.43 | 243.73 | -37.17 | 116.61 | 0.6505 | -742.0 | -573.1 | |
| 0.00 | 1.99 | 0.00 | 1.29 | -16.04 | 243.69 | -37.21 | 116.04 | 0.6491 | -836.0 | -647.4 | |
| 0.00 | 1.72 | 0.00 | 1.12 | -15.86 | 243.37 | -37.53 | 115.60 | 0.6520 | -921.0 | -821.2 | |
| 0.00 | 1.63 | 0.00 | 1.07 | -16.21 | 243.13 | -37.77 | 115.99 | 0.6565 | -657.0 | -446.7 | |
| 0.00 | 1.09 | 0.00 | 0.71 | -15.76 | 243.11 | -37.79 | 115.34 | 0.6547 | -849.0 | -750.5 | |
| 1.27 | 4.44 | 0.83 | 2.90 | -15.51 | 243.09 | -37.81 | 114.96 | 0.6539 | -795.7 | -688.3 | |
| 0.00 | 1.99 | 0.00 | 1.31 | -15.92 | 242.96 | -37.94 | 115.49 | 0.6573 | -693.0 | -633.1 | |
| 0.00 | 1.18 | 0.00 | 0.77 | -16.11 | 242.83 | -38.07 | 115.70 | 0.6596 | -581.0 | -449.5 | |
| 1.27 | 9.42 | 0.84 | 6.24 | -16.18 | 242.45 | -38.45 | 115.60 | 0.6644 | -682.9 | -650.1 | |
| 1.90 | -24.00 | 1.26 | -24.00 | -16.50 | 242.26 | -38.64 | 115.96 | 0.6682 | -726.0 | 999999 | |
| 0.00 | 1.72 | 0.00 | 1.14 | -15.74 | 242.27 | -38.63 | 114.88 | 0.6646 | -519.0 | -324.2 | |
| 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. | |