SDO HMI 2014-08-03 13:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.18 | 0.00 | 10.43 | 13.40 | 258.61 | 21.66 | 291.50 | 0.3909 | 152.3 | 82.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.18 | 0.00 | 0.70 | 13.61 | 270.37 | 33.42 | 285.67 | 0.5581 | -741.0 | -654.4 | |
| 0.00 | 2.26 | 0.00 | 1.34 | 14.07 | 269.96 | 33.01 | 286.61 | 0.5535 | -600.0 | -530.1 | |
| 0.00 | 1.45 | 0.00 | 0.84 | 15.86 | 267.66 | 30.71 | 290.77 | 0.5274 | -643.0 | -551.2 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 16.02 | 266.37 | 29.42 | 291.71 | 0.5101 | -676.0 | -542.1 | |
| 0.00 | 0.54 | 0.00 | 0.31 | 16.40 | 266.29 | 29.33 | 292.46 | 0.5105 | -734.0 | -575.2 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 12.42 | 265.60 | 28.65 | 284.98 | 0.4867 | -747.0 | -597.5 | |
| 0.00 | 1.00 | 0.00 | 0.53 | 9.33 | 259.40 | 22.45 | 280.07 | 0.3843 | 706.0 | 554.8 | |
| 0.00 | 1.18 | 0.00 | 0.63 | 14.35 | 258.79 | 21.84 | 293.07 | 0.3934 | 684.0 | 518.6 | |
| 0.00 | 0.72 | 0.00 | 0.39 | 17.73 | 257.85 | 20.90 | 301.82 | 0.4016 | 633.0 | 373.8 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 17.73 | 257.10 | 20.15 | 302.66 | 0.3914 | 572.0 | 449.7 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 8.32 | 251.23 | 14.27 | 280.40 | 0.2491 | 832.0 | 596.1 | |
| 0.00 | 0.54 | 0.00 | 0.28 | 17.53 | 250.05 | 13.09 | 313.30 | 0.2981 | 628.0 | 522.0 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 17.42 | 249.71 | 12.76 | 313.71 | 0.2928 | 778.0 | 577.6 | |
| 0.00 | 3.53 | 0.00 | 1.79 | 7.71 | 248.71 | 11.76 | 279.32 | 0.2056 | 766.0 | 496.9 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 23.57 | 243.68 | 6.72 | 340.52 | 0.3233 | 826.0 | 599.9 | |
| 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. | |