SDO HMI 2011-08-07 16:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.70 | 69.28 | 18.26 | 37.46 | -16.69 | 242.45 | -5.29 | 167.46 | 0.4014 | -14.2 | 155.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.71 | 0.00 | 1.44 | -14.75 | 246.29 | -1.45 | 176.08 | 0.3599 | 1232.0 | 965.3 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -15.86 | 245.81 | -1.93 | 175.06 | 0.3785 | 900.0 | 701.5 | |
| 0.00 | 2.08 | 0.00 | 1.11 | -16.00 | 245.55 | -2.19 | 174.45 | 0.3810 | 723.0 | 596.7 | |
| 1.99 | 5.24 | 1.06 | 2.79 | -15.28 | 245.34 | -2.40 | 173.70 | 0.3698 | 923.5 | 769.4 | |
| 0.00 | 1.99 | 0.00 | 1.06 | -15.77 | 244.83 | -2.91 | 172.55 | 0.3787 | 632.0 | 449.7 | |
| 9.76 | 21.23 | 5.26 | 11.45 | -16.67 | 243.89 | -3.85 | 170.60 | 0.3952 | 840.2 | 263.7 | |
| 4.97 | -6.00 | 2.68 | -6.00 | -16.90 | 243.82 | -3.92 | 170.53 | 0.3991 | -582.1 | 999999 | |
| 0.00 | 2.26 | 0.00 | 1.21 | -15.58 | 243.63 | -4.11 | 169.45 | 0.3787 | 961.0 | 665.2 | |
| 0.27 | -6.00 | 0.15 | -6.00 | -16.64 | 243.57 | -4.17 | 169.82 | 0.3956 | 721.3 | 999999 | |
| 0.00 | 0.72 | 0.00 | 0.39 | -16.50 | 243.39 | -4.35 | 169.31 | 0.3941 | 783.0 | 620.4 | |
| 0.00 | 2.62 | 0.00 | 1.41 | -16.28 | 242.91 | -4.82 | 168.06 | 0.3920 | 919.0 | 723.3 | |
| 0.00 | 2.17 | 0.00 | 1.18 | -16.99 | 241.27 | -6.47 | 164.66 | 0.4093 | -65.0 | -120.8 | |
| 0.00 | 2.98 | 0.00 | 1.62 | -17.03 | 240.59 | -7.15 | 163.19 | 0.4129 | -1017.0 | -914.7 | |
| 3.16 | 3.88 | 1.72 | 2.11 | -16.97 | 240.12 | -7.62 | 162.08 | 0.4143 | -984.3 | -775.4 | |
| 13.55 | 17.16 | 7.39 | 9.36 | -17.31 | 240.04 | -7.70 | 162.17 | 0.4197 | -929.2 | -669.3 | |
| 0.00 | 1.08 | 0.00 | 0.60 | -18.71 | 237.77 | -9.97 | 158.65 | 0.4524 | -729.0 | -553.3 | |
| 0.00 | 1.99 | 0.00 | 1.10 | -18.51 | 237.61 | -10.12 | 158.18 | 0.4504 | -878.0 | -624.1 | |
| 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. | |