SDO HMI 2011-10-13 15:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.42 | 28.84 | 3.05 | 16.51 | 21.04 | 110.23 | 26.72 | 302.61 | 0.5008 | 473.7 | 320.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.87 | 0.00 | 0.53 | 25.54 | 114.29 | 30.79 | 306.99 | 0.5804 | 338.0 | 383.1 | |
| 0.00 | 1.05 | 0.00 | 0.63 | 25.49 | 114.01 | 30.50 | 307.12 | 0.5768 | 687.0 | 574.0 | |
| 0.00 | 1.75 | 0.00 | 1.06 | 25.66 | 113.90 | 30.39 | 307.46 | 0.5767 | 782.0 | 712.9 | |
| 0.00 | 1.22 | 0.00 | 0.70 | 20.64 | 110.89 | 27.38 | 301.50 | 0.5068 | -914.0 | -758.1 | |
| 0.00 | 3.06 | 0.00 | 1.75 | 20.42 | 110.81 | 27.30 | 301.17 | 0.5045 | -960.0 | -779.7 | |
| 1.31 | 3.06 | 0.75 | 1.75 | 20.25 | 110.67 | 27.16 | 300.96 | 0.5015 | -938.3 | -672.8 | |
| 0.00 | 1.14 | 0.00 | 0.67 | 24.92 | 111.32 | 27.81 | 308.39 | 0.5420 | 687.0 | 484.1 | |
| 0.00 | 0.87 | 0.00 | 0.52 | 25.98 | 111.17 | 27.67 | 310.18 | 0.5485 | 829.0 | 674.6 | |
| 0.00 | 1.49 | 0.00 | 0.84 | 19.89 | 109.57 | 26.06 | 301.19 | 0.4850 | 660.0 | 511.6 | |
| 0.00 | 1.22 | 0.00 | 0.69 | 18.64 | 109.32 | 25.81 | 299.00 | 0.4737 | 850.0 | 676.3 | |
| 0.00 | 2.71 | 0.00 | 1.53 | 19.59 | 109.41 | 25.90 | 300.76 | 0.4809 | 958.0 | 789.3 | |
| 0.00 | 2.27 | 0.00 | 1.28 | 19.99 | 108.74 | 25.23 | 302.09 | 0.4748 | 1015.0 | 822.6 | |
| 2.71 | 6.73 | 1.52 | 3.77 | 19.53 | 108.63 | 25.12 | 301.31 | 0.4702 | 871.5 | 790.6 | |
| 0.00 | 1.40 | 0.00 | 0.79 | 20.21 | 108.71 | 25.20 | 302.53 | 0.4759 | 849.0 | 719.6 | |
| 1.40 | -13.00 | 0.78 | -13.00 | 19.54 | 108.42 | 24.91 | 301.51 | 0.4675 | 933.1 | 999999 | |
| 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. | |