SDO HMI 2011-06-07 01:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.33 | 140.83 | 13.30 | 71.15 | 9.35 | 336.82 | -6.38 | 33.93 | 0.1971 | -985.7 | -474.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.62 | 0.00 | 1.32 | 8.43 | 339.47 | -3.73 | 23.72 | 0.1607 | -748.0 | -659.0 | |
| 0.00 | 1.09 | 0.00 | 0.54 | 7.66 | 339.29 | -3.91 | 26.89 | 0.1500 | -831.0 | -682.5 | |
| 21.90 | 121.09 | 11.06 | 61.18 | 9.45 | 336.98 | -6.22 | 33.09 | 0.1966 | -1407.3 | -472.3 | |
| 1.99 | -3.00 | 1.01 | -3.00 | 9.20 | 336.65 | -6.55 | 35.20 | 0.1963 | -946.2 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 7.97 | 336.27 | -6.93 | 40.81 | 0.1838 | -1111.0 | -993.8 | |
| 2.44 | 3.44 | 1.23 | 1.74 | 8.62 | 336.16 | -7.04 | 39.00 | 0.1934 | -925.2 | -848.0 | |
| 0.00 | 0.90 | 0.00 | 0.46 | 8.13 | 336.17 | -7.03 | 40.65 | 0.1868 | -1102.0 | -957.1 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 8.03 | 336.02 | -7.18 | 41.58 | 0.1874 | -884.0 | -751.5 | |
| 0.00 | 1.54 | 0.00 | 0.78 | 10.59 | 335.37 | -7.83 | 36.10 | 0.2282 | -859.0 | -632.1 | |
| 0.00 | 1.63 | 0.00 | 0.82 | 8.25 | 335.27 | -7.93 | 43.63 | 0.1988 | -826.0 | -639.9 | |
| 0.00 | 2.81 | 0.00 | 1.42 | 9.42 | 334.81 | -8.39 | 41.38 | 0.2188 | -897.0 | -628.1 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 10.31 | 333.03 | -10.17 | 44.17 | 0.2504 | 962.0 | 705.1 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 10.16 | 332.91 | -10.29 | 44.95 | 0.2500 | 988.0 | 731.2 | |
| 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. | |