SDO HMI 2014-04-06 05:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.68 | 117.49 | 11.67 | 66.12 | 17.73 | 30.34 | 15.12 | 328.36 | 0.4760 | -320.4 | -243.2 | |
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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 | 0.48 | 10.71 | 33.84 | 18.62 | 312.35 | 0.4264 | 758.0 | 617.1 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 13.24 | 32.21 | 16.99 | 319.15 | 0.4368 | 709.0 | 491.8 | |
| 0.00 | 2.64 | 0.00 | 1.49 | 17.44 | 31.26 | 16.04 | 326.46 | 0.4791 | -903.0 | -736.2 | |
| 15.93 | 94.71 | 8.99 | 53.39 | 17.75 | 30.90 | 15.68 | 327.43 | 0.4801 | -1093.5 | -364.5 | |
| 4.75 | -4.00 | 2.68 | -4.00 | 17.68 | 30.60 | 15.38 | 327.84 | 0.4767 | -1238.5 | 999999 | |
| 0.00 | 5.63 | 0.00 | 3.18 | 18.32 | 30.20 | 14.98 | 329.25 | 0.4818 | -768.0 | -526.4 | |
| 0.00 | 0.70 | 0.00 | 0.40 | 19.19 | 27.76 | 12.54 | 334.36 | 0.4757 | 572.0 | 472.8 | |
| 0.00 | 1.94 | 0.00 | 1.09 | 19.05 | 27.62 | 12.40 | 334.47 | 0.4729 | 708.0 | 484.1 | |
| 0.00 | 2.02 | 0.00 | 1.12 | 17.49 | 27.08 | 11.86 | 333.91 | 0.4477 | 739.0 | 599.3 | |
| 0.00 | 0.53 | 0.00 | 0.29 | 17.53 | 25.96 | 10.74 | 336.12 | 0.4409 | 716.0 | 677.8 | |
| 0.00 | 1.41 | 0.00 | 0.78 | 17.63 | 25.87 | 10.65 | 336.39 | 0.4417 | 692.0 | 588.0 | |
| 0.00 | 2.73 | 0.00 | 1.50 | 17.49 | 25.74 | 10.52 | 336.53 | 0.4389 | 992.0 | 812.8 | |
| 0.00 | 2.02 | 0.00 | 1.13 | 19.72 | 24.68 | 9.46 | 340.48 | 0.4651 | 702.0 | 488.8 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 19.08 | 24.10 | 8.88 | 341.13 | 0.4527 | 649.0 | 503.8 | |
| 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. | |