SDO HMI 2011-06-02 03:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.08 | 172.40 | 19.94 | 103.52 | -20.54 | 19.39 | -28.88 | 127.14 | 0.5695 | 672.3 | 417.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.81 | 0.00 | 1.05 | -20.20 | 23.31 | -24.96 | 130.36 | 0.5219 | -740.0 | -692.8 | |
| 0.00 | 2.89 | 0.00 | 1.68 | -19.07 | 22.36 | -25.92 | 127.60 | 0.5234 | -685.0 | -597.6 | |
| 0.00 | 2.26 | 0.00 | 1.32 | -19.39 | 22.26 | -26.01 | 128.02 | 0.5271 | -873.0 | -723.6 | |
| 0.00 | 1.63 | 0.00 | 0.94 | -18.55 | 22.15 | -26.12 | 126.57 | 0.5217 | -885.0 | -548.1 | |
| 0.00 | 1.18 | 0.00 | 0.69 | -18.87 | 21.71 | -26.57 | 126.66 | 0.5296 | -795.0 | -617.6 | |
| 26.12 | 150.50 | 15.71 | 90.41 | -20.51 | 19.43 | -28.85 | 127.12 | 0.5689 | 1134.5 | 491.7 | |
| 4.70 | -6.00 | 2.85 | -6.00 | -20.83 | 18.76 | -29.51 | 127.03 | 0.5789 | 715.3 | 999999 | |
| 2.26 | 3.89 | 1.38 | 2.37 | -21.35 | 18.53 | -29.74 | 127.61 | 0.5853 | 704.2 | 529.8 | |
| 0.00 | 1.99 | 0.00 | 1.21 | -21.08 | 18.33 | -29.94 | 127.05 | 0.5857 | 688.0 | 578.0 | |
| 0.00 | 1.27 | 0.00 | 0.77 | -20.27 | 18.43 | -29.84 | 125.94 | 0.5787 | 616.0 | 487.1 | |
| 0.00 | 1.27 | 0.00 | 0.77 | -20.86 | 18.08 | -30.19 | 126.51 | 0.5869 | 580.0 | 490.6 | |
| 0.00 | 1.81 | 0.00 | 1.12 | -21.24 | 17.35 | -30.93 | 126.49 | 0.5980 | 735.0 | 600.8 | |
| 0.00 | 1.90 | 0.00 | 1.19 | -22.32 | 16.27 | -32.00 | 127.18 | 0.6175 | 655.0 | 467.9 | |
| 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. | |