SDO HMI 2011-11-11 16:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.79 | 334.94 | 33.31 | 190.33 | 28.07 | 44.17 | -16.35 | 30.51 | 0.4910 | -1024.7 | -390.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.03 | 0.00 | 0.57 | 27.97 | 49.27 | -11.25 | 22.38 | 0.4546 | -741.0 | -527.8 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 33.09 | 46.79 | -13.73 | 21.74 | 0.5388 | -657.0 | -457.8 | |
| 0.00 | 1.46 | 0.00 | 0.84 | 31.29 | 46.75 | -13.77 | 23.36 | 0.5151 | -873.0 | -763.0 | |
| 0.00 | 1.55 | 0.00 | 0.90 | 31.49 | 46.36 | -14.16 | 23.75 | 0.5201 | -675.0 | -576.8 | |
| 0.00 | 2.24 | 0.00 | 1.33 | 33.33 | 43.96 | -16.56 | 25.35 | 0.5584 | -767.0 | -553.0 | |
| 1.12 | 317.65 | 0.63 | 180.08 | 27.36 | 44.80 | -15.72 | 30.42 | 0.4773 | -1077.6 | -393.4 | |
| 55.60 | -6.00 | 31.50 | -6.00 | 27.88 | 44.30 | -16.22 | 30.56 | 0.4876 | -1278.7 | 999999 | |
| 2.07 | -6.00 | 1.18 | -6.00 | 28.53 | 44.02 | -16.50 | 30.21 | 0.4979 | -315.8 | 999999 | |
| 0.00 | 1.89 | 0.00 | 1.18 | 36.55 | 41.60 | -18.92 | 25.30 | 0.6117 | -739.0 | -685.6 | |
| 0.00 | 1.12 | 0.00 | 0.64 | 28.39 | 41.92 | -18.60 | 33.31 | 0.5130 | -748.0 | -577.5 | |
| 0.00 | 2.50 | 0.00 | 1.45 | 28.98 | 41.49 | -19.03 | 33.18 | 0.5234 | -735.0 | -669.7 | |
| 0.00 | 1.29 | 0.00 | 0.76 | 27.61 | 38.38 | -22.14 | 38.78 | 0.5353 | 677.0 | 465.9 | |
| 0.00 | 1.55 | 0.00 | 0.96 | 30.19 | 34.32 | -26.21 | 39.83 | 0.5982 | 559.0 | 361.1 | |
| 0.00 | 1.46 | 0.00 | 0.91 | 30.29 | 34.02 | -26.50 | 40.00 | 0.6017 | 627.0 | 449.5 | |
| 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. | |