SDO HMI 2014-08-21 19:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.25 | 160.72 | 15.60 | 95.02 | 16.41 | 27.96 | 32.29 | 289.71 | 0.5463 | -713.4 | -336.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.00 | 134.45 | 14.27 | 80.00 | 16.24 | 28.65 | 32.98 | 289.07 | 0.5551 | -1185.5 | -342.3 | |
| 1.62 | -1.00 | 0.96 | -1.00 | 16.36 | 28.22 | 32.55 | 289.44 | 0.5496 | -1154.0 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 17.00 | 26.48 | 30.81 | 291.33 | 0.5279 | -782.0 | -545.3 | |
| 0.63 | 2.79 | 0.37 | 1.63 | 17.55 | 26.55 | 30.87 | 292.31 | 0.5309 | -838.9 | -706.9 | |
| 0.00 | 1.08 | 0.00 | 0.62 | 14.11 | 25.82 | 30.15 | 286.14 | 0.5091 | -637.0 | -515.2 | |
| 0.00 | 2.43 | 0.00 | 1.41 | 17.42 | 26.15 | 30.48 | 292.26 | 0.5250 | -679.0 | -612.6 | |
| 0.00 | 9.89 | 0.00 | 5.72 | 17.22 | 25.82 | 30.15 | 292.06 | 0.5197 | -730.0 | -713.9 | |
| 0.00 | 1.62 | 0.00 | 0.93 | 16.78 | 24.83 | 29.16 | 291.74 | 0.5042 | -746.0 | -574.5 | |
| 0.00 | 1.98 | 0.00 | 1.11 | 18.59 | 21.79 | 26.12 | 297.16 | 0.4709 | 655.0 | 545.1 | |
| 0.00 | 1.71 | 0.00 | 0.94 | 17.30 | 20.35 | 24.68 | 295.57 | 0.4438 | 796.0 | 679.5 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 18.95 | 20.29 | 24.61 | 299.05 | 0.4525 | 786.0 | 693.2 | |
| 0.00 | 1.62 | 0.00 | 0.89 | 16.71 | 19.78 | 24.11 | 294.73 | 0.4325 | 793.0 | 657.9 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 17.19 | 18.91 | 23.24 | 296.46 | 0.4228 | 743.0 | 632.0 | |
| 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. | |