SDO HMI 2014-04-23 09:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.82 | 383.56 | 33.30 | 216.87 | 17.79 | 166.52 | 17.95 | 322.51 | 0.4838 | -689.3 | -314.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.96 | 353.76 | 32.26 | 200.36 | 17.76 | 166.89 | 18.32 | 321.86 | 0.4866 | -1394.6 | -410.6 | |
| 1.42 | -1.00 | 0.80 | -1.00 | 17.67 | 166.25 | 17.68 | 322.73 | 0.4797 | -1108.3 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 18.12 | 163.22 | 14.65 | 328.26 | 0.4588 | 560.0 | 495.6 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 18.28 | 162.94 | 14.37 | 328.94 | 0.4586 | 784.0 | 680.3 | |
| 0.00 | 1.24 | 0.00 | 0.70 | 19.20 | 162.96 | 14.38 | 329.98 | 0.4708 | 691.0 | 570.6 | |
| 0.00 | 1.07 | 0.00 | 0.59 | 18.28 | 162.74 | 14.17 | 329.28 | 0.4570 | 695.0 | 538.9 | |
| 0.00 | 9.33 | 0.00 | 5.18 | 18.02 | 162.69 | 14.12 | 329.07 | 0.4531 | 788.0 | 809.1 | |
| 0.00 | 1.16 | 0.00 | 0.65 | 19.07 | 162.78 | 14.21 | 330.13 | 0.4677 | 636.0 | 502.2 | |
| 0.00 | 1.78 | 0.00 | 0.99 | 18.67 | 162.61 | 14.04 | 329.97 | 0.4611 | 723.0 | 615.5 | |
| 0.00 | 1.60 | 0.00 | 0.89 | 18.93 | 162.60 | 14.03 | 330.28 | 0.4645 | 771.0 | 610.1 | |
| 0.00 | 0.89 | 0.00 | 0.50 | 20.06 | 162.64 | 14.07 | 331.45 | 0.4797 | 571.0 | 483.3 | |
| 0.00 | 1.87 | 0.00 | 1.05 | 19.99 | 162.33 | 13.76 | 331.90 | 0.4765 | 625.0 | 642.9 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 17.60 | 161.55 | 12.98 | 330.66 | 0.4386 | 622.0 | 467.5 | |
| 0.00 | 1.16 | 0.00 | 0.63 | 17.40 | 161.43 | 12.86 | 330.63 | 0.4351 | 921.0 | 755.2 | |
| 0.00 | 3.47 | 0.00 | 1.90 | 17.20 | 161.29 | 12.72 | 330.67 | 0.4313 | 782.0 | 615.7 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 17.50 | 161.28 | 12.71 | 331.04 | 0.4352 | 860.0 | 749.9 | |
| 0.44 | 1.33 | 0.24 | 0.73 | 17.16 | 160.42 | 11.85 | 332.32 | 0.4240 | 863.6 | 728.9 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 17.45 | 160.44 | 11.86 | 332.61 | 0.4282 | 795.0 | 582.2 | |
| 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. | |