SDO HMI 2011-08-25 16:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.03 | 0.00 | 12.44 | 16.36 | 329.37 | -40.44 | 73.02 | 0.6523 | -205.4 | -80.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.17 | 0.00 | 0.70 | 13.77 | 335.22 | -34.59 | 75.91 | 0.5707 | -756.0 | -693.2 | |
| 0.00 | 0.99 | 0.00 | 0.60 | 13.92 | 335.08 | -34.73 | 75.69 | 0.5729 | -743.0 | -626.4 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 13.51 | 334.92 | -34.89 | 76.44 | 0.5743 | -574.0 | -393.0 | |
| 0.00 | 1.79 | 0.00 | 1.10 | 14.53 | 333.70 | -36.11 | 74.96 | 0.5929 | -711.0 | -506.9 | |
| 0.00 | 0.90 | 0.00 | 0.57 | 17.54 | 331.70 | -38.11 | 70.60 | 0.6262 | -819.0 | -723.2 | |
| 0.00 | 2.06 | 0.00 | 1.33 | 18.50 | 330.42 | -39.39 | 69.48 | 0.6448 | -635.0 | -506.9 | |
| 0.00 | 1.44 | 0.00 | 0.95 | 18.74 | 328.63 | -41.18 | 69.62 | 0.6675 | -650.0 | -457.9 | |
| 0.00 | 1.17 | 0.00 | 0.78 | 18.34 | 328.32 | -41.49 | 70.29 | 0.6703 | -588.0 | -451.5 | |
| 0.00 | 0.99 | 0.00 | 0.66 | 18.17 | 328.20 | -41.61 | 70.57 | 0.6714 | -492.0 | -345.2 | |
| 0.00 | 1.70 | 0.00 | 1.15 | 16.10 | 327.19 | -42.62 | 73.82 | 0.6797 | 589.0 | 521.8 | |
| 0.00 | 0.90 | 0.00 | 0.61 | 16.00 | 326.70 | -43.11 | 74.06 | 0.6855 | 622.0 | 572.4 | |
| 0.00 | 2.06 | 0.00 | 1.41 | 16.66 | 326.43 | -43.38 | 73.15 | 0.6898 | 746.0 | 649.2 | |
| 0.00 | 1.26 | 0.00 | 0.86 | 15.19 | 325.83 | -43.98 | 75.37 | 0.6950 | 592.0 | 473.4 | |
| 0.00 | 1.70 | 0.00 | 1.18 | 15.82 | 325.62 | -44.20 | 74.49 | 0.6984 | 543.0 | 391.6 | |
| 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. | |