SDO HMI 2011-04-29 15:59:06 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.58 | 35.90 | 6.01 | 18.63 | -18.02 | 120.90 | -10.44 | 144.11 | 0.2951 | -38.5 | -81.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.98 | 0.00 | 0.51 | -19.10 | 124.51 | -6.84 | 156.20 | 0.2801 | 749.0 | 613.0 | |
| 0.00 | 1.16 | 0.00 | 0.60 | -17.15 | 122.51 | -8.84 | 146.59 | 0.2678 | 1068.0 | 755.9 | |
| 0.00 | 1.07 | 0.00 | 0.55 | -17.37 | 122.44 | -8.91 | 146.83 | 0.2714 | 931.0 | 787.6 | |
| 0.00 | 2.05 | 0.00 | 1.05 | -16.87 | 122.40 | -8.95 | 145.64 | 0.2650 | 970.0 | 934.5 | |
| 0.00 | 1.25 | 0.00 | 0.64 | -18.17 | 122.33 | -9.02 | 148.18 | 0.2836 | 814.0 | 605.9 | |
| 0.00 | 0.98 | 0.00 | 0.51 | -18.36 | 122.29 | -9.06 | 148.42 | 0.2866 | 934.0 | 665.5 | |
| 0.00 | 2.49 | 0.00 | 1.28 | -17.02 | 122.26 | -9.09 | 145.59 | 0.2684 | 764.0 | 834.3 | |
| 0.00 | 1.16 | 0.00 | 0.60 | -17.15 | 122.13 | -9.22 | 145.47 | 0.2713 | 922.0 | 825.7 | |
| 0.00 | 1.16 | 0.00 | 0.60 | -17.05 | 121.65 | -9.69 | 143.92 | 0.2746 | -801.0 | -621.8 | |
| 4.28 | 12.91 | 2.21 | 6.70 | -17.46 | 120.31 | -11.04 | 141.35 | 0.2937 | -1043.1 | -870.7 | |
| 5.61 | -10.00 | 2.91 | -10.00 | -17.77 | 120.13 | -11.22 | 141.59 | 0.2994 | -1048.5 | 999999 | |
| 1.69 | 9.00 | 0.89 | 4.71 | -19.45 | 119.98 | -11.36 | 144.67 | 0.3226 | -978.1 | -832.8 | |
| 0.00 | 1.69 | 0.00 | 0.88 | -17.37 | 120.06 | -11.29 | 140.52 | 0.2951 | -740.0 | -651.9 | |
| 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. | |