SDO HMI 2014-04-06 23:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 82.81 | 433.13 | 43.82 | 229.33 | 12.70 | 13.50 | 8.18 | 336.75 | 0.3534 | -1014.0 | -376.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.94 | 0.00 | 1.04 | 14.24 | 15.13 | 9.81 | 334.61 | 0.3868 | 690.0 | 577.9 | |
| 0.00 | 1.32 | 0.00 | 0.71 | 14.44 | 13.73 | 8.41 | 338.07 | 0.3807 | 687.0 | 470.2 | |
| 79.99 | 415.18 | 42.33 | 219.82 | 12.65 | 13.60 | 8.28 | 336.45 | 0.3532 | -1346.8 | -401.7 | |
| 2.82 | -3.00 | 1.49 | -3.00 | 13.32 | 13.28 | 7.96 | 337.99 | 0.3611 | -926.2 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.69 | 9.90 | 12.54 | 7.21 | 335.92 | 0.3045 | 622.0 | 536.3 | |
| 0.00 | 1.58 | 0.00 | 0.83 | 11.43 | 11.83 | 6.51 | 339.82 | 0.3237 | -635.0 | -586.6 | |
| 0.00 | 1.50 | 0.00 | 0.80 | 15.28 | 11.69 | 6.37 | 343.69 | 0.3828 | 819.0 | 625.4 | |
| 0.00 | 1.32 | 0.00 | 0.70 | 14.51 | 11.45 | 6.13 | 343.69 | 0.3697 | -704.0 | -622.1 | |
| 0.00 | 2.02 | 0.00 | 1.08 | 14.51 | 11.27 | 5.94 | 344.16 | 0.3688 | -950.0 | -773.7 | |
| 0.00 | 0.88 | 0.00 | 0.46 | 12.37 | 11.12 | 5.79 | 342.78 | 0.3346 | -566.0 | -463.6 | |
| 0.00 | 1.67 | 0.00 | 0.88 | 12.50 | 11.06 | 5.74 | 343.06 | 0.3363 | -513.0 | -419.7 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 14.56 | 10.08 | 4.76 | 347.22 | 0.3649 | 723.0 | 537.2 | |
| 0.00 | 1.85 | 0.00 | 0.98 | 14.27 | 9.27 | 3.95 | 349.20 | 0.3575 | 870.0 | 661.5 | |
| 0.00 | 1.67 | 0.00 | 0.87 | 11.41 | 8.85 | 3.53 | 348.71 | 0.3098 | 744.0 | 588.3 | |
| 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. | |