SDO HMI 2011-08-10 02:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.66 | 0.00 | 12.16 | 19.30 | 224.05 | 8.28 | 329.29 | 0.2649 | -358.4 | -321.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.08 | 0.00 | 1.08 | 20.00 | 226.70 | 10.92 | 323.16 | 0.2983 | -965.0 | -762.2 | |
| 0.00 | 0.63 | 0.00 | 0.33 | 20.33 | 226.06 | 10.29 | 325.42 | 0.2964 | -786.0 | -674.7 | |
| 0.00 | 1.54 | 0.00 | 0.79 | 19.55 | 225.98 | 10.20 | 323.99 | 0.2852 | -794.0 | -645.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 20.46 | 225.58 | 9.80 | 326.94 | 0.2937 | -723.0 | -552.7 | |
| 0.00 | 3.25 | 0.00 | 1.68 | 20.03 | 225.48 | 9.71 | 326.31 | 0.2869 | -854.0 | -795.7 | |
| 0.00 | 1.99 | 0.00 | 1.03 | 20.22 | 225.13 | 9.36 | 327.64 | 0.2864 | -833.0 | -650.1 | |
| 0.00 | 1.44 | 0.00 | 0.74 | 19.11 | 224.51 | 8.74 | 327.07 | 0.2654 | -810.0 | -673.5 | |
| 0.00 | 1.81 | 0.00 | 0.92 | 18.05 | 224.30 | 8.53 | 325.32 | 0.2488 | -1014.0 | -865.4 | |
| 0.00 | 1.08 | 0.00 | 0.55 | 18.15 | 223.88 | 8.11 | 326.86 | 0.2463 | -756.0 | -565.8 | |
| 0.00 | 2.26 | 0.00 | 1.16 | 18.71 | 223.55 | 7.78 | 329.17 | 0.2513 | -758.0 | -678.1 | |
| 0.00 | 1.35 | 0.00 | 0.69 | 19.30 | 221.96 | 6.19 | 335.62 | 0.2475 | 668.0 | 505.7 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 18.90 | 221.56 | 5.78 | 336.33 | 0.2385 | 661.0 | 463.7 | |
| 0.00 | 2.62 | 0.00 | 1.34 | 19.21 | 221.41 | 5.63 | 337.41 | 0.2424 | 1132.0 | 841.1 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 18.07 | 220.66 | 4.89 | 338.26 | 0.2197 | 815.0 | 688.5 | |
| 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. | |