SDO HMI 2014-06-06 15:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.04 | 0.00 | 9.52 | 4.58 | 258.33 | -25.06 | 78.37 | 0.4271 | -35.4 | 9.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.55 | 4.92 | 273.56 | -9.84 | 63.17 | 0.1916 | -1051.0 | -853.0 | |
| 0.00 | 1.72 | 0.00 | 0.87 | 5.23 | 273.49 | -9.91 | 61.92 | 0.1950 | -976.0 | -739.4 | |
| 0.00 | 1.18 | 0.00 | 0.60 | 2.31 | 270.10 | -13.29 | 80.00 | 0.2343 | -820.0 | -650.0 | |
| 0.00 | 1.72 | 0.00 | 0.88 | 1.09 | 267.88 | -15.52 | 85.86 | 0.2694 | -908.0 | -616.3 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 2.43 | 266.79 | -16.60 | 81.49 | 0.2899 | -823.0 | -649.1 | |
| 0.00 | 0.90 | 0.00 | 0.47 | -2.16 | 266.41 | -16.99 | 97.30 | 0.2956 | -766.0 | -599.6 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 1.16 | 261.61 | -21.78 | 86.83 | 0.3732 | 738.0 | 494.6 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 3.76 | 253.84 | -29.55 | 82.38 | 0.4985 | 722.0 | 583.4 | |
| 0.00 | 1.09 | 0.00 | 0.64 | 8.20 | 251.97 | -31.42 | 74.52 | 0.5375 | 574.0 | 487.5 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 6.03 | 249.44 | -33.95 | 79.27 | 0.5674 | 624.0 | 515.4 | |
| 0.00 | 0.45 | 0.00 | 0.28 | 9.40 | 248.73 | -34.67 | 73.74 | 0.5868 | 552.0 | 604.2 | |
| 0.00 | 1.99 | 0.00 | 1.22 | 9.71 | 248.31 | -35.08 | 73.39 | 0.5934 | 426.0 | 426.1 | |
| 0.00 | 1.09 | 0.00 | 0.67 | 9.28 | 248.32 | -35.07 | 74.10 | 0.5918 | 595.0 | 468.2 | |
| 0.00 | 1.00 | 0.00 | 0.67 | -0.61 | 240.83 | -42.56 | 90.88 | 0.6787 | 617.0 | 523.8 | |
| 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. | |