SDO HMI 2014-08-21 17:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.84 | 27.51 | 6.20 | 24.31 | 15.80 | 53.15 | 56.37 | 284.50 | 0.8281 | 84.9 | -5.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.97 | 4.67 | 3.03 | 4.77 | 14.77 | 58.52 | 61.74 | 283.09 | 0.8763 | -611.7 | -431.9 | |
| 0.00 | 0.27 | 0.00 | 0.27 | 14.41 | 58.34 | 61.56 | 282.68 | 0.8749 | -503.0 | -415.7 | |
| 0.00 | 1.17 | 0.00 | 1.10 | 16.38 | 55.60 | 58.82 | 285.02 | 0.8519 | -329.0 | -306.7 | |
| 0.00 | 4.94 | 0.00 | 4.57 | 15.98 | 54.98 | 58.20 | 284.57 | 0.8463 | -706.0 | -577.3 | |
| 0.00 | 0.63 | 0.00 | 0.56 | 16.44 | 53.19 | 56.41 | 285.20 | 0.8300 | -321.0 | -316.4 | |
| 0.00 | 1.62 | 0.00 | 1.37 | 15.34 | 51.38 | 54.60 | 283.95 | 0.8122 | 412.0 | 324.6 | |
| 0.00 | 1.62 | 0.00 | 1.36 | 14.96 | 51.07 | 54.29 | 283.51 | 0.8090 | 539.0 | 512.8 | |
| 1.08 | 2.52 | 0.91 | 2.11 | 15.74 | 51.05 | 54.27 | 284.48 | 0.8091 | 529.0 | 356.9 | |
| 0.00 | 0.81 | 0.00 | 0.67 | 14.95 | 50.53 | 53.75 | 283.52 | 0.8036 | 534.0 | 440.3 | |
| 0.00 | 1.08 | 0.00 | 0.88 | 16.23 | 49.85 | 53.07 | 285.17 | 0.7974 | 436.0 | 339.7 | |
| 2.79 | 4.49 | 2.26 | 3.64 | 15.95 | 49.48 | 52.70 | 284.85 | 0.7935 | 597.0 | 459.7 | |
| 0.00 | 1.26 | 0.00 | 1.04 | 18.61 | 50.22 | 53.44 | 288.11 | 0.8031 | 345.0 | 289.6 | |
| 0.00 | 0.72 | 0.00 | 0.57 | 13.52 | 48.29 | 51.51 | 281.82 | 0.7797 | 546.0 | 466.6 | |
| 0.00 | 1.71 | 0.00 | 1.40 | 18.27 | 49.80 | 53.02 | 287.73 | 0.7986 | 530.0 | 396.2 | |
| 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. | |