SDO HMI 2014-04-23 16:02:05 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.59 | 394.94 | 32.28 | 229.00 | 17.83 | 166.54 | 21.83 | 317.08 | 0.5219 | -795.8 | -320.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.59 | 372.56 | 32.28 | 216.25 | 17.78 | 166.77 | 22.06 | 316.70 | 0.5236 | -1359.7 | -388.8 | |
| 0.00 | 1.42 | 0.00 | 0.81 | 17.58 | 164.61 | 19.90 | 319.32 | 0.4997 | 442.0 | 385.9 | |
| 0.00 | 4.35 | 0.00 | 2.47 | 17.93 | 162.97 | 18.26 | 322.16 | 0.4880 | 952.0 | 799.0 | |
| 0.00 | 1.07 | 0.00 | 0.61 | 18.22 | 162.91 | 18.19 | 322.64 | 0.4908 | 752.0 | 622.2 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 18.58 | 162.91 | 18.20 | 323.10 | 0.4951 | 641.0 | 545.1 | |
| 0.00 | 1.69 | 0.00 | 0.96 | 17.99 | 162.71 | 18.00 | 322.63 | 0.4862 | 945.0 | 770.6 | |
| 0.00 | 2.84 | 0.00 | 1.62 | 18.87 | 162.68 | 17.97 | 323.82 | 0.4964 | 562.0 | 585.6 | |
| 0.00 | 1.78 | 0.00 | 1.01 | 18.44 | 162.63 | 17.92 | 323.35 | 0.4909 | 745.0 | 714.7 | |
| 0.00 | 0.89 | 0.00 | 0.51 | 19.83 | 162.65 | 17.94 | 325.03 | 0.5076 | 628.0 | 530.0 | |
| 0.00 | 1.86 | 0.00 | 1.07 | 20.06 | 162.38 | 17.67 | 325.71 | 0.5080 | 704.0 | 705.9 | |
| 0.00 | 1.95 | 0.00 | 1.11 | 18.46 | 162.13 | 17.42 | 324.13 | 0.4866 | 840.0 | 752.2 | |
| 0.00 | 2.22 | 0.00 | 1.28 | 20.38 | 162.18 | 17.47 | 326.39 | 0.5103 | 592.0 | 542.3 | |
| 0.00 | 1.33 | 0.00 | 0.74 | 17.09 | 160.54 | 15.83 | 324.91 | 0.4555 | 847.0 | 682.5 | |
| 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. | |