SDO HMI 2011-07-04 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 |
| 38.31 | 231.92 | 20.60 | 124.20 | 16.72 | 354.40 | 17.94 | 308.93 | 0.3801 | -498.0 | -325.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.68 | 14.56 | 356.72 | 20.26 | 300.82 | 0.3920 | -776.0 | -602.1 | |
| 0.00 | 0.82 | 0.00 | 0.45 | 18.23 | 356.51 | 20.05 | 308.84 | 0.4198 | -818.0 | -593.7 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 16.92 | 356.15 | 19.70 | 306.65 | 0.4036 | 65.0 | 84.9 | |
| 1.63 | 189.04 | 0.88 | 101.59 | 16.55 | 355.74 | 19.28 | 306.41 | 0.3950 | -696.6 | -431.2 | |
| 3.45 | -4.00 | 1.86 | -4.00 | 16.36 | 355.59 | 19.13 | 306.22 | 0.3914 | -1034.8 | 999999 | |
| 0.00 | 1.82 | 0.00 | 0.97 | 15.27 | 355.38 | 18.92 | 304.08 | 0.3793 | -705.0 | -390.5 | |
| 23.06 | -4.00 | 12.41 | -4.00 | 16.68 | 355.35 | 18.89 | 307.22 | 0.3912 | -1329.4 | 999999 | |
| 0.00 | 0.73 | 0.00 | 0.39 | 14.16 | 354.88 | 18.43 | 302.14 | 0.3635 | -711.0 | -536.2 | |
| 10.17 | -4.00 | 5.45 | -4.00 | 16.82 | 354.73 | 18.27 | 308.39 | 0.3845 | -1270.0 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 18.59 | 354.17 | 17.71 | 312.85 | 0.3950 | -560.0 | -523.8 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 14.59 | 353.43 | 16.97 | 305.22 | 0.3473 | -856.0 | -635.3 | |
| 0.00 | 1.73 | 0.00 | 0.94 | 20.88 | 354.06 | 17.60 | 317.27 | 0.4181 | -595.0 | -462.9 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 19.71 | 353.79 | 17.33 | 315.58 | 0.4023 | -627.0 | -447.9 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 19.52 | 353.73 | 17.27 | 315.31 | 0.3997 | -843.0 | -578.6 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 19.75 | 353.15 | 16.69 | 316.68 | 0.3957 | -817.0 | -620.6 | |
| 0.00 | 1.91 | 0.00 | 1.02 | 20.18 | 352.01 | 15.55 | 319.39 | 0.3884 | -864.0 | -703.3 | |
| 0.00 | 2.36 | 0.00 | 1.26 | 19.10 | 351.70 | 15.25 | 317.95 | 0.3726 | -529.0 | -497.0 | |
| 0.00 | 0.64 | 0.00 | 0.34 | 20.00 | 350.98 | 14.53 | 320.93 | 0.3756 | -836.0 | -691.4 | |
| 0.00 | 0.82 | 0.00 | 0.43 | 19.28 | 350.72 | 14.26 | 320.10 | 0.3641 | -650.0 | -533.2 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 15.76 | 349.98 | 13.52 | 314.16 | 0.3151 | 838.0 | 623.4 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 12.41 | 349.75 | 13.29 | 305.67 | 0.2776 | 698.0 | 541.3 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 19.70 | 350.12 | 13.67 | 322.04 | 0.3631 | -883.0 | -642.8 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 15.98 | 349.67 | 13.21 | 315.33 | 0.3140 | 959.0 | 894.2 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 16.49 | 349.41 | 12.96 | 317.03 | 0.3168 | 786.0 | 712.2 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 16.65 | 349.29 | 12.84 | 317.65 | 0.3173 | 925.0 | 717.8 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 15.99 | 349.15 | 12.69 | 316.46 | 0.3080 | 832.0 | 686.3 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 14.50 | 348.86 | 12.41 | 313.40 | 0.2876 | 785.0 | 560.6 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 16.81 | 348.46 | 12.00 | 319.87 | 0.3102 | 901.0 | 721.4 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 16.94 | 348.20 | 11.75 | 320.74 | 0.3091 | 844.0 | 671.5 | |
| 0.00 | 2.63 | 0.00 | 1.37 | 16.82 | 348.03 | 11.58 | 320.87 | 0.3057 | 990.0 | 675.7 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 17.07 | 347.56 | 11.11 | 322.55 | 0.3041 | 889.0 | 749.0 | |
| 0.00 | 2.91 | 0.00 | 1.49 | 13.03 | 347.03 | 10.57 | 313.76 | 0.2487 | 976.0 | 787.6 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 17.42 | 347.22 | 10.77 | 324.09 | 0.3053 | 812.0 | 670.6 | |
| 0.00 | 1.18 | 0.00 | 0.62 | 18.37 | 346.83 | 10.37 | 326.91 | 0.3143 | 836.0 | 645.2 | |
| 0.00 | 1.73 | 0.00 | 0.87 | 11.43 | 342.82 | 6.36 | 322.79 | 0.1804 | -806.0 | -616.9 | |
| 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. | |