SDO HMI 2011-06-04 17:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.02 | 239.29 | 24.04 | 125.16 | 17.32 | 19.88 | 5.78 | 342.28 | 0.3216 | -405.6 | -279.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.81 | 0.00 | 0.44 | 20.74 | 24.72 | 10.62 | 334.33 | 0.3995 | -675.0 | -622.4 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 19.99 | 22.31 | 8.21 | 338.83 | 0.3730 | -846.0 | -650.5 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 19.73 | 22.30 | 8.19 | 338.59 | 0.3690 | -720.0 | -625.8 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 19.57 | 22.16 | 8.05 | 338.75 | 0.3658 | -618.0 | -618.3 | |
| 26.67 | 184.24 | 13.93 | 96.23 | 16.78 | 21.16 | 7.06 | 338.13 | 0.3173 | -1289.9 | -477.6 | |
| 0.00 | 1.90 | 0.00 | 1.00 | 18.76 | 21.11 | 7.01 | 340.49 | 0.3475 | -926.0 | -681.9 | |
| 6.15 | -5.00 | 3.22 | -5.00 | 17.19 | 21.02 | 6.92 | 339.03 | 0.3228 | -1023.5 | 999999 | |
| 5.15 | -5.00 | 2.69 | -5.00 | 17.06 | 20.60 | 6.49 | 340.06 | 0.3184 | -1084.6 | 999999 | |
| 0.00 | 2.98 | 0.00 | 1.55 | 16.71 | 20.30 | 6.19 | 340.52 | 0.3113 | -321.0 | -430.9 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 20.15 | 18.44 | 4.34 | 348.50 | 0.3577 | -680.0 | -532.9 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 17.44 | 17.48 | 3.37 | 349.55 | 0.3109 | -854.0 | -622.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 17.32 | 17.35 | 3.24 | 349.87 | 0.3084 | -817.0 | -626.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 17.83 | 16.49 | 2.39 | 352.72 | 0.3146 | -714.0 | -352.6 | |
| 2.08 | 2.89 | 1.09 | 1.51 | 18.15 | 16.46 | 2.36 | 352.94 | 0.3199 | -866.2 | -754.9 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 19.73 | 15.39 | 1.28 | 356.47 | 0.3442 | 766.0 | 655.6 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 19.40 | 15.13 | 1.02 | 357.13 | 0.3386 | 820.0 | 616.9 | |
| 0.00 | 0.99 | 0.00 | 0.52 | 19.82 | 15.00 | 0.90 | 357.54 | 0.3455 | 782.0 | 634.3 | |
| 0.00 | 2.62 | 0.00 | 1.37 | 18.40 | 14.86 | 0.76 | 357.74 | 0.3219 | 912.0 | 807.1 | |
| 0.00 | 1.90 | 0.00 | 1.00 | 19.11 | 14.87 | 0.76 | 357.82 | 0.3337 | 1079.0 | 861.4 | |
| 3.71 | 10.49 | 1.94 | 5.49 | 18.60 | 14.58 | 0.47 | 358.61 | 0.3250 | 1100.7 | 910.5 | |
| 2.26 | 6.15 | 1.17 | 3.20 | 17.25 | 14.41 | 0.31 | 359.01 | 0.3026 | 1142.9 | 827.6 | |
| 0.00 | 3.16 | 0.00 | 1.65 | 18.11 | 14.42 | 0.31 | 359.06 | 0.3169 | 1012.0 | 798.9 | |
| 0.00 | 4.07 | 0.00 | 2.13 | 18.76 | 14.13 | 0.02 | 359.93 | 0.3276 | 979.0 | 714.3 | |
| 0.00 | 1.18 | 0.00 | 0.64 | 23.53 | 13.63 | -0.47 | 1.07 | 0.4054 | 771.0 | 636.2 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 18.98 | 13.58 | -0.52 | 1.50 | 0.3314 | 826.0 | 648.1 | |
| 0.00 | 1.72 | 0.00 | 0.93 | 23.00 | 13.40 | -0.70 | 1.63 | 0.3970 | 627.0 | 472.4 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 22.83 | 13.24 | -0.87 | 2.03 | 0.3944 | 734.0 | 533.6 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 18.44 | 13.17 | -0.94 | 2.77 | 0.3226 | 843.0 | 601.8 | |
| 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. | |