SDO HMI 2014-08-23 18:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.84 | 38.18 | 3.03 | 19.92 | -10.23 | 332.46 | 2.66 | 189.02 | 0.3117 | 506.0 | 520.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.80 | 0.00 | 0.96 | -10.55 | 342.42 | 12.62 | 215.75 | 0.3693 | 814.0 | 545.7 | |
| 0.00 | 2.33 | 0.00 | 1.22 | -8.61 | 339.35 | 9.55 | 211.56 | 0.3148 | 821.0 | 633.0 | |
| 0.00 | 2.69 | 0.00 | 1.39 | -8.16 | 335.08 | 5.28 | 199.26 | 0.2773 | 1017.0 | 893.1 | |
| 5.84 | 14.10 | 3.03 | 7.31 | -9.63 | 333.99 | 4.19 | 194.16 | 0.2957 | 1077.7 | 800.8 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -5.73 | 332.79 | 3.00 | 193.30 | 0.2270 | 912.0 | 694.8 | |
| 0.00 | 4.40 | 0.00 | 2.37 | -16.16 | 332.45 | 2.65 | 186.45 | 0.3971 | 1054.0 | 830.9 | |
| 0.00 | 0.72 | 0.00 | 0.38 | -13.67 | 331.95 | 2.15 | 185.91 | 0.3561 | -640.0 | -584.9 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -8.38 | 331.92 | 2.12 | 187.87 | 0.2685 | 811.0 | 560.8 | |
| 0.00 | 2.96 | 0.00 | 1.52 | -8.50 | 330.39 | 0.59 | 182.18 | 0.2683 | 759.0 | 621.0 | |
| 0.00 | 1.08 | 0.00 | 0.56 | -10.81 | 330.17 | 0.37 | 181.20 | 0.3069 | 717.0 | 530.5 | |
| 0.00 | 0.99 | 0.00 | 0.51 | -10.78 | 330.02 | 0.22 | 180.71 | 0.3064 | 951.0 | 776.7 | |
| 0.00 | 0.63 | 0.00 | 0.32 | -6.21 | 329.78 | -0.02 | 179.91 | 0.2293 | 894.0 | 723.7 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -9.82 | 323.83 | -5.97 | 160.44 | 0.3075 | -998.0 | -836.1 | |
| 0.00 | 1.53 | 0.00 | 0.78 | -6.84 | 323.45 | -6.35 | 155.24 | 0.2635 | -974.0 | -687.8 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -14.70 | 316.10 | -13.70 | 147.97 | 0.4337 | -786.0 | -580.2 | |
| 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. | |