SDO HMI 2014-04-06 22:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79.01 | 428.59 | 41.76 | 226.59 | 12.69 | 13.50 | 7.62 | 338.18 | 0.3498 | -1056.3 | -392.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.61 | 12.10 | 15.47 | 9.60 | 332.48 | 0.3543 | 633.0 | 476.0 | |
| 1.58 | 410.82 | 0.84 | 217.22 | 13.06 | 13.83 | 7.95 | 337.73 | 0.3572 | -712.7 | -410.6 | |
| 77.43 | -2.00 | 40.92 | -2.00 | 12.67 | 13.60 | 7.72 | 337.90 | 0.3500 | -1409.0 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 11.45 | 11.93 | 6.05 | 341.17 | 0.3215 | -776.0 | -676.9 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 14.86 | 11.83 | 5.95 | 344.40 | 0.3744 | -592.0 | -393.7 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 15.31 | 11.62 | 5.75 | 345.23 | 0.3805 | 623.0 | 533.3 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 11.07 | 11.46 | 5.58 | 342.16 | 0.3130 | 727.0 | 476.3 | |
| 0.00 | 4.31 | 0.00 | 2.29 | 14.50 | 11.29 | 5.41 | 345.50 | 0.3665 | -832.0 | -631.7 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 12.42 | 11.09 | 5.21 | 344.47 | 0.3328 | -669.0 | -593.6 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 14.50 | 11.07 | 5.20 | 346.06 | 0.3656 | -680.0 | -576.4 | |
| 0.00 | 1.14 | 0.00 | 0.59 | 10.99 | 9.68 | 3.80 | 347.58 | 0.3041 | 747.0 | 561.0 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 13.72 | 9.66 | 3.78 | 349.34 | 0.3482 | 716.0 | 535.7 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 14.26 | 9.27 | 3.39 | 350.69 | 0.3558 | 793.0 | 721.0 | |
| 0.00 | 1.76 | 0.00 | 0.90 | 8.31 | 9.01 | 3.13 | 347.83 | 0.2576 | 778.0 | 556.0 | |
| 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. | |