SDO HMI 2011-06-13 12:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.79 | 38.90 | 4.12 | 20.61 | -15.36 | 244.63 | -13.12 | 141.93 | 0.3555 | -101.4 | -9.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.82 | 0.00 | 0.43 | -14.69 | 247.90 | -9.85 | 148.18 | 0.3153 | 821.0 | 612.8 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -15.61 | 247.47 | -10.28 | 148.65 | 0.3319 | 989.0 | 866.0 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -15.48 | 247.02 | -10.73 | 147.36 | 0.3340 | 785.0 | 617.3 | |
| 3.08 | 15.86 | 1.62 | 8.34 | -14.63 | 245.98 | -11.77 | 143.39 | 0.3325 | 1134.2 | 685.3 | |
| 1.54 | -4.00 | 0.81 | -4.00 | -14.70 | 245.75 | -12.00 | 142.98 | 0.3356 | 940.8 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.57 | -14.86 | 245.13 | -12.62 | 141.90 | 0.3439 | 527.0 | 474.8 | |
| 0.00 | 2.17 | 0.00 | 1.16 | -15.91 | 243.86 | -13.89 | 141.18 | 0.3699 | -824.0 | -601.9 | |
| 0.00 | 1.18 | 0.00 | 0.63 | -16.10 | 243.71 | -14.04 | 141.23 | 0.3738 | -824.0 | -652.9 | |
| 3.17 | 6.62 | 1.69 | 3.52 | -15.62 | 243.49 | -14.26 | 139.94 | 0.3703 | -1007.2 | -868.4 | |
| 0.00 | 2.45 | 0.00 | 1.31 | -16.58 | 243.05 | -14.70 | 140.80 | 0.3864 | -713.0 | -624.1 | |
| 0.00 | 2.36 | 0.00 | 1.26 | -15.94 | 243.00 | -14.75 | 139.60 | 0.3792 | -842.0 | -631.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -15.78 | 242.49 | -15.26 | 138.36 | 0.3828 | -814.0 | -642.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -15.69 | 242.11 | -15.64 | 137.50 | 0.3859 | -774.0 | -584.1 | |
| 0.00 | 1.36 | 0.00 | 0.74 | -17.19 | 241.35 | -16.40 | 138.81 | 0.4113 | -762.0 | -572.1 | |
| 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. | |