SDO HMI 2014-08-22 21:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.05 | 124.99 | 13.91 | 90.06 | 16.61 | 27.89 | 46.54 | 286.40 | 0.7267 | -342.0 | -207.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.05 | 106.01 | 13.91 | 77.56 | 16.43 | 28.80 | 47.45 | 285.96 | 0.7373 | -997.0 | -306.9 | |
| 0.00 | 1.53 | 0.00 | 1.08 | 18.38 | 26.81 | 45.46 | 288.96 | 0.7175 | -608.0 | -525.5 | |
| 0.00 | 0.90 | 0.00 | 0.63 | 17.20 | 25.98 | 44.63 | 287.46 | 0.7058 | -601.0 | -527.8 | |
| 0.00 | 1.35 | 0.00 | 0.92 | 16.53 | 25.11 | 43.76 | 286.66 | 0.6944 | -87.0 | -114.7 | |
| 0.00 | 0.36 | 0.00 | 0.24 | 18.02 | 22.82 | 41.46 | 289.31 | 0.6695 | -319.0 | -408.2 | |
| 0.00 | 3.59 | 0.00 | 2.36 | 17.66 | 21.87 | 40.51 | 289.01 | 0.6570 | 717.0 | 555.4 | |
| 0.00 | 1.62 | 0.00 | 1.06 | 17.80 | 21.65 | 40.30 | 289.28 | 0.6547 | 468.0 | 420.8 | |
| 0.00 | 1.44 | 0.00 | 0.94 | 18.08 | 21.57 | 40.21 | 289.73 | 0.6543 | 605.0 | 490.3 | |
| 0.00 | 1.08 | 0.00 | 0.70 | 18.16 | 21.38 | 40.03 | 289.90 | 0.6522 | 541.0 | 455.1 | |
| 0.00 | 0.72 | 0.00 | 0.47 | 17.93 | 21.15 | 39.79 | 289.61 | 0.6487 | 611.0 | 539.2 | |
| 0.00 | 1.62 | 0.00 | 1.05 | 18.76 | 21.30 | 39.94 | 290.83 | 0.6527 | 602.0 | 502.6 | |
| 0.00 | 1.08 | 0.00 | 0.69 | 16.78 | 20.27 | 38.92 | 288.08 | 0.6350 | 679.0 | 546.9 | |
| 0.00 | 1.44 | 0.00 | 0.93 | 18.85 | 20.57 | 39.22 | 291.18 | 0.6440 | 654.0 | 526.8 | |
| 0.00 | 1.35 | 0.00 | 0.86 | 16.68 | 20.00 | 38.65 | 287.98 | 0.6313 | 355.0 | 340.4 | |
| 0.00 | 0.90 | 0.00 | 0.57 | 17.46 | 19.91 | 38.56 | 289.23 | 0.6320 | 706.0 | 642.2 | |
| 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. | |