SDO HMI 2011-06-04 04:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.54 | 27.42 | 0.88 | 15.30 | 17.80 | 41.83 | 20.58 | 313.49 | 0.4594 | 96.1 | -85.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.54 | 0.00 | 0.90 | 20.61 | 46.64 | 25.39 | 311.64 | 0.5390 | 727.0 | 501.9 | |
| 1.54 | 6.15 | 0.88 | 3.52 | 17.92 | 45.32 | 24.06 | 308.86 | 0.5003 | -956.0 | -752.4 | |
| 0.00 | 1.81 | 0.00 | 1.03 | 18.05 | 45.09 | 23.84 | 309.32 | 0.4987 | -892.0 | -661.8 | |
| 0.00 | 1.63 | 0.00 | 0.92 | 16.45 | 44.32 | 23.07 | 307.49 | 0.4755 | -853.0 | -674.7 | |
| 0.00 | 3.62 | 0.00 | 2.06 | 18.66 | 44.41 | 23.16 | 311.09 | 0.4963 | -654.0 | -599.0 | |
| 0.00 | 1.18 | 0.00 | 0.66 | 18.17 | 43.30 | 22.05 | 311.62 | 0.4790 | -855.0 | -635.4 | |
| 0.00 | 0.99 | 0.00 | 0.56 | 18.46 | 43.20 | 21.95 | 312.22 | 0.4806 | -859.0 | -730.8 | |
| 0.00 | 1.09 | 0.00 | 0.59 | 16.82 | 39.14 | 17.88 | 315.06 | 0.4179 | 599.0 | 511.9 | |
| 0.00 | 2.53 | 0.00 | 1.37 | 16.88 | 37.32 | 16.06 | 318.15 | 0.3985 | 908.0 | 725.2 | |
| 0.00 | 1.90 | 0.00 | 1.02 | 16.34 | 36.91 | 15.65 | 317.91 | 0.3878 | 931.0 | 812.0 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 16.91 | 36.03 | 14.78 | 320.51 | 0.3853 | 700.0 | 497.3 | |
| 0.00 | 0.45 | 0.00 | 0.24 | 18.51 | 35.90 | 14.65 | 323.38 | 0.4037 | 886.0 | 843.4 | |
| 0.00 | 1.63 | 0.00 | 0.87 | 16.59 | 35.55 | 14.29 | 320.87 | 0.3765 | 963.0 | 780.8 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 18.38 | 35.43 | 14.17 | 324.06 | 0.3976 | 574.0 | 366.4 | |
| 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. | |