SDO HMI 2011-07-01 06:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.82 | 42.43 | 7.51 | 21.57 | 15.62 | 24.52 | 1.74 | 351.48 | 0.2271 | -260.8 | -24.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.36 | 0.00 | 1.23 | 20.03 | 27.29 | 4.51 | 345.96 | 0.3057 | -780.0 | -641.4 | |
| 8.09 | 14.54 | 4.08 | 7.34 | 13.34 | 26.56 | 3.78 | 340.58 | 0.1938 | 1112.8 | 798.0 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 15.34 | 25.24 | 2.46 | 349.17 | 0.2209 | -940.0 | -696.0 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.56 | 25.11 | 2.33 | 349.89 | 0.2242 | -911.0 | -703.0 | |
| 0.00 | 0.91 | 0.00 | 0.46 | 15.71 | 25.05 | 2.27 | 350.27 | 0.2267 | -1008.0 | -841.0 | |
| 1.64 | 3.73 | 0.83 | 1.90 | 16.37 | 24.84 | 2.06 | 351.62 | 0.2372 | -996.2 | -759.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 15.90 | 24.71 | 1.92 | 351.86 | 0.2289 | -984.0 | -784.3 | |
| 0.00 | 2.45 | 0.00 | 1.24 | 14.41 | 24.44 | 1.66 | 352.03 | 0.2030 | -985.0 | -791.5 | |
| 2.91 | 3.18 | 1.48 | 1.61 | 15.37 | 24.16 | 1.38 | 353.88 | 0.2188 | -1057.2 | -1062.3 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 16.81 | 23.44 | 0.66 | 357.38 | 0.2424 | -1034.0 | -771.4 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 17.41 | 22.61 | -0.17 | 0.64 | 0.2523 | -945.0 | -706.7 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 17.86 | 21.43 | -1.35 | 4.96 | 0.2608 | -645.0 | -370.5 | |
| 0.00 | 1.27 | 0.00 | 0.65 | 17.98 | 21.36 | -1.42 | 5.15 | 0.2630 | 499.0 | 457.3 | |
| 2.18 | 7.27 | 1.12 | 3.72 | 17.54 | 20.82 | -1.96 | 7.33 | 0.2566 | 908.5 | 844.8 | |
| 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. | |