SDO HMI 2014-04-15 08:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47.68 | 286.03 | 25.10 | 150.45 | 12.13 | 262.96 | 8.18 | 335.56 | 0.3386 | -790.1 | -327.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.12 | 0.00 | 1.13 | 12.22 | 265.92 | 11.15 | 328.14 | 0.3596 | 963.0 | 830.6 | |
| 28.13 | 270.64 | 14.82 | 142.38 | 12.21 | 263.67 | 8.90 | 333.61 | 0.3416 | -1335.0 | -392.5 | |
| 7.34 | -2.00 | 3.86 | -2.00 | 11.90 | 263.51 | 8.73 | 333.61 | 0.3357 | -1522.1 | 999999 | |
| 12.21 | -2.00 | 6.42 | -2.00 | 12.02 | 263.20 | 8.42 | 334.58 | 0.3353 | -1551.2 | 999999 | |
| 0.00 | 1.33 | 0.00 | 0.69 | 12.41 | 255.24 | 0.46 | 358.54 | 0.3105 | 584.0 | 432.3 | |
| 0.00 | 1.50 | 0.00 | 0.79 | 13.55 | 254.53 | -0.25 | 0.73 | 0.3294 | 786.0 | 606.1 | |
| 0.00 | 1.86 | 0.00 | 0.96 | 11.15 | 254.53 | -0.25 | 0.84 | 0.2893 | 840.0 | 694.0 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 13.11 | 254.44 | -0.34 | 1.03 | 0.3220 | 956.0 | 786.2 | |
| 0.00 | 1.50 | 0.00 | 0.78 | 12.07 | 251.88 | -2.89 | 9.24 | 0.3086 | 816.0 | 642.2 | |
| 0.00 | 1.77 | 0.00 | 0.91 | 9.68 | 248.84 | -5.93 | 21.18 | 0.2832 | 700.0 | 522.4 | |
| 0.00 | 1.06 | 0.00 | 0.57 | 16.58 | 248.55 | -6.22 | 15.41 | 0.3926 | 819.0 | 637.5 | |
| 0.00 | 1.42 | 0.00 | 0.74 | 12.04 | 246.57 | -8.21 | 24.82 | 0.3340 | 783.0 | 576.9 | |
| 0.00 | 1.86 | 0.00 | 0.99 | 13.78 | 244.79 | -9.99 | 27.03 | 0.3723 | 640.0 | 425.4 | |
| 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. | |