SDO HMI 2011-06-12 06:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.03 | 50.57 | 11.06 | 29.74 | -15.75 | 245.92 | -28.36 | 121.83 | 0.5382 | 99.1 | 3.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.81 | 4.17 | 1.03 | 2.36 | -15.42 | 249.94 | -24.34 | 124.77 | 0.4856 | 943.0 | 698.7 | |
| 4.44 | 19.21 | 2.52 | 10.90 | -15.42 | 249.63 | -24.65 | 124.45 | 0.4896 | 915.8 | 776.3 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -15.67 | 249.52 | -24.75 | 124.79 | 0.4929 | 612.0 | 410.1 | |
| 7.16 | -2.00 | 4.06 | -2.00 | -15.07 | 249.46 | -24.82 | 123.67 | 0.4889 | 904.7 | 999999 | |
| 0.00 | 2.27 | 0.00 | 1.33 | -15.47 | 246.09 | -28.19 | 121.26 | 0.5347 | 860.0 | 689.0 | |
| 0.00 | 0.63 | 0.00 | 0.37 | -14.56 | 244.75 | -29.53 | 118.68 | 0.5459 | 576.0 | 577.6 | |
| 0.00 | 1.18 | 0.00 | 0.70 | -14.91 | 244.66 | -29.62 | 119.19 | 0.5492 | 612.0 | 479.6 | |
| 0.00 | 1.72 | 0.00 | 1.04 | -15.65 | 243.15 | -31.13 | 119.27 | 0.5729 | -888.0 | -708.7 | |
| 0.00 | 1.72 | 0.00 | 1.04 | -15.93 | 242.84 | -31.44 | 119.51 | 0.5785 | -863.0 | -760.3 | |
| 0.00 | 2.63 | 0.00 | 1.60 | -15.68 | 242.21 | -32.07 | 118.68 | 0.5848 | -881.0 | -724.9 | |
| 0.00 | 1.36 | 0.00 | 0.83 | -16.13 | 242.09 | -32.19 | 119.29 | 0.5889 | -933.0 | -798.3 | |
| 5.62 | 10.24 | 3.45 | 6.30 | -16.64 | 241.92 | -32.36 | 119.96 | 0.5941 | -931.0 | -585.4 | |
| 0.00 | 0.73 | 0.00 | 0.44 | -15.85 | 241.88 | -32.40 | 118.71 | 0.5899 | -290.0 | -235.4 | |
| 0.00 | 3.26 | 0.00 | 2.01 | -16.80 | 241.66 | -32.61 | 120.03 | 0.5982 | -458.0 | -449.2 | |
| 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. | |