SDO HMI 2011-07-05 08:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.24 | 289.72 | 27.46 | 163.67 | 16.97 | 354.36 | 25.62 | 300.47 | 0.4811 | -384.0 | -217.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.00 | 0.00 | 0.59 | 19.08 | 358.53 | 29.79 | 300.72 | 0.5482 | -636.0 | -482.5 | |
| 0.00 | 1.73 | 0.00 | 1.00 | 17.59 | 357.22 | 28.48 | 299.14 | 0.5224 | 372.0 | 452.6 | |
| 0.00 | 1.36 | 0.00 | 0.79 | 18.16 | 357.14 | 28.40 | 300.20 | 0.5249 | 496.0 | 412.7 | |
| 36.07 | 222.61 | 20.56 | 126.63 | 16.82 | 355.58 | 26.84 | 299.00 | 0.4961 | -1133.6 | -365.6 | |
| 9.99 | -4.00 | 5.66 | -4.00 | 16.90 | 354.78 | 26.03 | 299.81 | 0.4859 | -1169.9 | 999999 | |
| 1.18 | -4.00 | 0.67 | -4.00 | 16.97 | 354.29 | 25.55 | 300.36 | 0.4800 | -858.5 | 999999 | |
| 0.00 | 5.36 | 0.00 | 3.07 | 19.59 | 354.49 | 25.75 | 304.93 | 0.5012 | -715.0 | -573.2 | |
| 0.00 | 2.09 | 0.00 | 1.17 | 16.99 | 353.80 | 25.05 | 300.82 | 0.4735 | -799.0 | -672.5 | |
| 1.00 | 3.27 | 0.57 | 1.85 | 18.28 | 353.89 | 25.14 | 303.15 | 0.4838 | 938.6 | 729.4 | |
| 0.00 | 2.54 | 0.00 | 1.41 | 15.56 | 352.87 | 24.13 | 298.87 | 0.4516 | -760.0 | -729.2 | |
| 0.00 | 2.45 | 0.00 | 1.36 | 15.94 | 352.75 | 24.00 | 299.75 | 0.4524 | -712.0 | -739.4 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 16.57 | 352.83 | 24.09 | 300.91 | 0.4578 | -483.0 | -396.2 | |
| 0.00 | 0.82 | 0.00 | 0.46 | 18.08 | 352.94 | 24.19 | 303.69 | 0.4701 | 765.0 | 586.3 | |
| 0.00 | 2.09 | 0.00 | 1.16 | 16.42 | 352.53 | 23.79 | 300.90 | 0.4527 | -746.0 | -561.2 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 16.30 | 352.27 | 23.53 | 300.91 | 0.4484 | -828.0 | -664.8 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 19.34 | 351.75 | 23.01 | 307.25 | 0.4652 | -745.0 | -577.9 | |
| 0.00 | 2.82 | 0.00 | 1.57 | 19.12 | 351.68 | 22.94 | 306.92 | 0.4626 | -861.0 | -730.1 | |
| 0.00 | 3.09 | 0.00 | 1.68 | 15.97 | 350.04 | 21.29 | 302.57 | 0.4160 | 814.0 | 664.6 | |
| 0.00 | 3.82 | 0.00 | 2.07 | 15.38 | 349.87 | 21.12 | 301.49 | 0.4092 | 818.0 | 636.0 | |
| 0.00 | 1.36 | 0.00 | 0.76 | 19.72 | 350.34 | 21.59 | 309.57 | 0.4513 | -761.0 | -625.4 | |
| 0.00 | 3.36 | 0.00 | 1.83 | 16.23 | 349.79 | 21.05 | 303.39 | 0.4147 | 736.0 | 633.2 | |
| 0.00 | 1.45 | 0.00 | 0.80 | 19.16 | 349.88 | 21.13 | 309.10 | 0.4407 | -738.0 | -579.8 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 16.51 | 349.42 | 20.67 | 304.43 | 0.4121 | 806.0 | 650.4 | |
| 0.00 | 2.27 | 0.00 | 1.24 | 16.95 | 349.47 | 20.72 | 305.28 | 0.4163 | 587.0 | 509.5 | |
| 0.00 | 4.54 | 0.00 | 2.47 | 16.86 | 349.28 | 20.54 | 305.32 | 0.4132 | 798.0 | 725.9 | |
| 0.00 | 0.91 | 0.00 | 0.49 | 16.68 | 349.23 | 20.49 | 304.99 | 0.4110 | 1004.0 | 897.4 | |
| 0.00 | 5.45 | 0.00 | 2.95 | 17.55 | 347.80 | 19.06 | 308.66 | 0.4004 | 1009.0 | 786.0 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 17.12 | 347.55 | 18.81 | 308.10 | 0.3932 | 833.0 | 688.2 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 17.81 | 347.36 | 18.61 | 309.82 | 0.3973 | 889.0 | 763.0 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 17.12 | 347.22 | 18.47 | 308.59 | 0.3890 | 850.0 | 648.0 | |
| 0.00 | 1.73 | 0.00 | 0.93 | 18.11 | 346.75 | 18.00 | 311.30 | 0.3927 | 862.0 | 692.2 | |
| 0.00 | 1.54 | 0.00 | 0.83 | 18.17 | 346.52 | 17.77 | 311.78 | 0.3906 | 903.0 | 743.4 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 17.26 | 346.29 | 17.55 | 310.25 | 0.3788 | 882.0 | 731.6 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 16.82 | 346.21 | 17.47 | 309.43 | 0.3736 | 739.0 | 657.7 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 16.89 | 345.99 | 17.24 | 309.92 | 0.3714 | 944.0 | 832.7 | |
| 0.00 | 0.36 | 0.00 | 0.20 | 18.88 | 346.09 | 17.34 | 313.84 | 0.3927 | 816.0 | 769.2 | |
| 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. | |