SDO HMI 2014-04-08 20:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.29 | 356.07 | 38.30 | 222.62 | 12.72 | 13.29 | 32.71 | 300.15 | 0.6117 | -846.8 | -344.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.56 | 13.92 | 14.72 | 34.14 | 300.78 | 0.6363 | 613.0 | 530.0 | |
| 0.00 | 2.38 | 0.00 | 1.48 | 10.98 | 14.10 | 33.51 | 297.00 | 0.6106 | -767.0 | -580.4 | |
| 55.75 | 331.05 | 34.89 | 207.32 | 12.73 | 13.42 | 32.84 | 300.06 | 0.6134 | -1259.6 | -383.6 | |
| 0.53 | 1.41 | 0.32 | 0.86 | 10.38 | 12.93 | 32.34 | 296.93 | 0.5924 | 583.0 | 446.4 | |
| 1.14 | 4.67 | 0.70 | 2.86 | 10.68 | 12.67 | 32.09 | 297.57 | 0.5911 | 706.2 | 424.1 | |
| 2.20 | -3.00 | 1.38 | -3.00 | 13.34 | 12.93 | 32.34 | 301.30 | 0.6115 | -880.4 | 999999 | |
| 0.00 | 2.47 | 0.00 | 1.56 | 14.78 | 13.13 | 32.54 | 303.19 | 0.6237 | 661.0 | 437.8 | |
| 0.00 | 0.88 | 0.00 | 0.54 | 13.12 | 11.95 | 31.37 | 301.77 | 0.5985 | -603.0 | -421.9 | |
| 0.44 | 1.50 | 0.27 | 0.91 | 12.11 | 11.38 | 30.80 | 300.74 | 0.5846 | -728.2 | -619.2 | |
| 0.00 | 1.41 | 0.00 | 0.86 | 12.87 | 11.37 | 30.79 | 301.87 | 0.5898 | -691.0 | -628.4 | |
| 1.23 | 2.73 | 0.74 | 1.65 | 11.85 | 10.56 | 29.98 | 301.02 | 0.5728 | 557.5 | 401.4 | |
| 0.00 | 1.67 | 0.00 | 1.01 | 12.51 | 10.58 | 29.99 | 302.01 | 0.5777 | 433.0 | 220.1 | |
| 0.00 | 1.06 | 0.00 | 0.63 | 12.34 | 9.81 | 29.23 | 302.42 | 0.5672 | 614.0 | 505.5 | |
| 0.00 | 1.23 | 0.00 | 0.74 | 11.96 | 9.66 | 29.07 | 301.97 | 0.5625 | 116.0 | 160.1 | |
| 0.00 | 1.59 | 0.00 | 0.96 | 13.67 | 9.67 | 29.08 | 304.53 | 0.5755 | 706.0 | 517.6 | |
| 0.00 | 1.14 | 0.00 | 0.68 | 14.37 | 7.90 | 27.32 | 307.25 | 0.5606 | 735.0 | 596.7 | |
| 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. | |