SDO HMI 2011-11-14 06:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.00 | 58.25 | 33.20 | 60.37 | 19.48 | 87.14 | 60.69 | 290.62 | 0.8800 | -157.5 | -78.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.86 | 0.00 | 0.94 | 18.97 | 89.05 | 62.60 | 289.79 | 0.8941 | -385.0 | -336.9 | |
| 6.88 | 21.25 | 7.55 | 23.15 | 19.32 | 89.00 | 62.55 | 290.18 | 0.8941 | -497.2 | -329.0 | |
| 5.33 | -2.00 | 5.74 | -2.00 | 19.25 | 88.41 | 61.96 | 290.18 | 0.8897 | -740.5 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.89 | 18.62 | 87.09 | 60.64 | 289.64 | 0.8790 | -492.0 | -414.1 | |
| 8.26 | 12.73 | 8.25 | 12.71 | 18.30 | 86.08 | 59.63 | 289.41 | 0.8705 | 562.8 | 309.5 | |
| 1.63 | 2.50 | 1.65 | 2.51 | 19.29 | 86.22 | 59.77 | 290.52 | 0.8728 | 267.0 | 203.4 | |
| 0.00 | 0.69 | 0.00 | 0.68 | 18.71 | 85.82 | 59.37 | 289.92 | 0.8689 | -553.0 | -389.6 | |
| 0.00 | 2.15 | 0.00 | 2.19 | 19.96 | 86.51 | 60.06 | 291.24 | 0.8759 | 339.0 | 186.7 | |
| 0.00 | 0.86 | 0.00 | 0.86 | 19.83 | 85.93 | 59.47 | 291.18 | 0.8710 | 328.0 | 194.1 | |
| 0.00 | 0.69 | 0.00 | 0.67 | 18.52 | 85.16 | 58.71 | 289.80 | 0.8632 | 441.0 | 365.9 | |
| 0.00 | 0.52 | 0.00 | 0.52 | 20.31 | 85.85 | 59.39 | 291.73 | 0.8710 | 347.0 | 273.8 | |
| 7.92 | 10.58 | 8.10 | 10.83 | 21.32 | 86.45 | 60.00 | 292.79 | 0.8770 | -594.5 | -415.5 | |
| 0.00 | 1.12 | 0.00 | 1.08 | 18.87 | 84.93 | 58.48 | 290.24 | 0.8618 | 420.0 | 311.6 | |
| 1.98 | 2.75 | 1.91 | 2.66 | 19.70 | 84.62 | 58.17 | 291.24 | 0.8602 | 303.8 | 356.3 | |
| 0.00 | 0.69 | 0.00 | 0.68 | 20.83 | 85.25 | 58.80 | 292.44 | 0.8669 | 63.0 | 105.4 | |
| 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. | |