SDO HMI 2011-06-03 18:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.49 | 27.20 | 5.23 | 14.80 | 17.43 | 42.97 | 16.19 | 319.64 | 0.4087 | -177.3 | -81.8 | |
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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 | 0.65 | 15.82 | 47.01 | 20.22 | 309.98 | 0.4359 | 807.0 | 610.8 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 16.96 | 45.78 | 19.00 | 313.74 | 0.4328 | -698.0 | -516.6 | |
| 6.87 | 11.39 | 3.79 | 6.28 | 17.95 | 45.55 | 18.77 | 315.77 | 0.4406 | -882.9 | -990.8 | |
| 2.62 | -3.00 | 1.44 | -3.00 | 18.05 | 45.32 | 18.54 | 316.27 | 0.4392 | -867.3 | 999999 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 16.32 | 44.18 | 17.40 | 315.04 | 0.4078 | -824.0 | -613.1 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 18.75 | 44.36 | 17.57 | 318.90 | 0.4367 | -608.0 | -574.6 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 18.33 | 43.01 | 16.22 | 320.42 | 0.4180 | -907.0 | -778.8 | |
| 0.00 | 1.17 | 0.00 | 0.63 | 17.53 | 42.07 | 15.29 | 320.73 | 0.3989 | 865.0 | 683.8 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 17.30 | 41.75 | 14.97 | 320.93 | 0.3930 | -823.0 | -635.9 | |
| 0.00 | 0.99 | 0.00 | 0.53 | 16.63 | 41.07 | 14.29 | 321.05 | 0.3779 | -800.0 | -676.0 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 16.82 | 37.77 | 10.98 | 328.34 | 0.3490 | 807.0 | 520.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 16.63 | 37.30 | 10.52 | 329.12 | 0.3424 | 829.0 | 628.0 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 16.47 | 36.81 | 10.03 | 330.06 | 0.3361 | 888.0 | 627.2 | |
| 0.00 | 0.81 | 0.00 | 0.43 | 16.28 | 36.22 | 9.44 | 331.23 | 0.3286 | 826.0 | 547.0 | |
| 0.00 | 1.17 | 0.00 | 0.62 | 16.31 | 35.74 | 8.96 | 332.51 | 0.3253 | 1001.0 | 773.4 | |
| 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. | |