SDO HMI 2011-05-28 11:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.02 | 43.02 | 10.80 | 22.09 | -15.76 | 113.71 | 3.66 | 193.37 | 0.2637 | -403.3 | -280.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.98 | 3.97 | 1.54 | 2.05 | -15.66 | 118.49 | 8.45 | 209.40 | 0.2894 | 889.0 | 652.2 | |
| 0.00 | 1.26 | 0.00 | 0.65 | -15.34 | 118.45 | 8.40 | 209.83 | 0.2845 | 850.0 | 687.3 | |
| 0.00 | 1.26 | 0.00 | 0.65 | -15.40 | 118.29 | 8.24 | 209.26 | 0.2841 | 834.0 | 725.8 | |
| 0.00 | 1.44 | 0.00 | 0.74 | -15.10 | 116.57 | 6.52 | 204.42 | 0.2663 | 1028.0 | 722.1 | |
| 0.00 | 0.63 | 0.00 | 0.33 | -15.82 | 116.37 | 6.32 | 202.66 | 0.2761 | 784.0 | 583.0 | |
| 0.00 | 0.90 | 0.00 | 0.46 | -15.98 | 115.64 | 5.59 | 200.08 | 0.2741 | 855.0 | 678.0 | |
| 0.00 | 1.35 | 0.00 | 0.69 | -15.82 | 113.77 | 3.72 | 193.83 | 0.2624 | -836.0 | -653.8 | |
| 0.00 | 1.80 | 0.00 | 0.93 | -15.95 | 113.55 | 3.50 | 192.93 | 0.2636 | -958.0 | -778.9 | |
| 0.00 | 2.44 | 0.00 | 1.25 | -15.32 | 113.48 | 3.43 | 193.24 | 0.2530 | -843.0 | -438.4 | |
| 1.44 | 3.70 | 0.74 | 1.90 | -15.95 | 112.89 | 2.84 | 190.54 | 0.2613 | -942.1 | -781.9 | |
| 5.32 | 6.77 | 2.73 | 3.47 | -15.85 | 112.60 | 2.55 | 189.56 | 0.2589 | -1188.8 | -937.2 | |
| 11.28 | 13.08 | 5.79 | 6.72 | -16.26 | 112.54 | 2.49 | 189.09 | 0.2655 | -1008.4 | -717.2 | |
| 0.00 | 1.80 | 0.00 | 0.91 | -12.61 | 111.04 | 0.99 | 184.84 | 0.2006 | -962.0 | -769.7 | |
| 0.00 | 2.62 | 0.00 | 1.34 | -15.92 | 111.05 | 1.00 | 183.78 | 0.2569 | -728.0 | -582.0 | |
| 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. | |