SDO HMI 2011-02-11 23:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 25.32 | 0.00 | 14.08 | 20.21 | 63.97 | 1.64 | 356.60 | 0.4569 | 338.3 | 242.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.71 | 0.00 | 0.96 | 19.68 | 70.23 | 7.91 | 343.70 | 0.4634 | -846.0 | -675.0 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 18.03 | 69.56 | 7.23 | 343.98 | 0.4358 | -664.0 | -539.3 | |
| 0.00 | 2.22 | 0.00 | 1.26 | 22.27 | 66.61 | 4.29 | 351.86 | 0.4907 | -817.0 | -665.5 | |
| 0.00 | 3.25 | 0.00 | 1.81 | 20.35 | 65.13 | 2.81 | 354.23 | 0.4585 | -756.0 | -605.2 | |
| 0.00 | 1.80 | 0.00 | 0.99 | 19.38 | 64.27 | 1.94 | 355.84 | 0.4423 | 689.0 | 525.0 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 19.64 | 63.86 | 1.54 | 356.74 | 0.4460 | 729.0 | 533.7 | |
| 0.00 | 0.60 | 0.00 | 0.33 | 18.56 | 63.66 | 1.34 | 357.02 | 0.4288 | 657.0 | 496.4 | |
| 0.00 | 1.88 | 0.00 | 1.04 | 19.71 | 62.86 | 0.53 | 358.87 | 0.4464 | 956.0 | 818.5 | |
| 0.00 | 3.51 | 0.00 | 1.94 | 19.91 | 62.70 | 0.38 | 359.21 | 0.4495 | 948.0 | 754.4 | |
| 0.00 | 2.14 | 0.00 | 1.19 | 20.21 | 62.64 | 0.31 | 359.35 | 0.4541 | 866.0 | 757.8 | |
| 0.00 | 1.28 | 0.00 | 0.71 | 20.40 | 62.64 | 0.31 | 359.36 | 0.4572 | 852.0 | 707.0 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 20.60 | 62.04 | -0.29 | 0.59 | 0.4603 | 688.0 | 534.7 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 20.94 | 60.42 | -1.90 | 3.83 | 0.4665 | 700.0 | 548.9 | |
| 0.00 | 2.22 | 0.00 | 1.24 | 20.94 | 60.20 | -2.13 | 4.27 | 0.4668 | 734.0 | 553.8 | |
| 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. | |