SDO HMI 2014-04-09 22:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.70 | 0.00 | 9.97 | -14.75 | 299.82 | -26.46 | 111.92 | 0.4654 | -375.8 | -371.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.41 | 0.00 | 0.75 | -19.94 | 310.94 | -15.34 | 134.47 | 0.3501 | 29.0 | 28.5 | |
| 0.00 | 1.67 | 0.00 | 0.87 | -15.43 | 310.85 | -15.43 | 123.09 | 0.3075 | 560.0 | 483.8 | |
| 0.00 | 0.71 | 0.00 | 0.37 | -19.38 | 309.50 | -16.78 | 130.83 | 0.3614 | 706.0 | 608.9 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -10.31 | 306.15 | -20.13 | 103.47 | 0.3498 | -7.0 | -1.8 | |
| 0.00 | 2.20 | 0.00 | 1.23 | -15.53 | 299.81 | -26.47 | 112.27 | 0.4661 | -733.0 | -576.9 | |
| 0.00 | 1.41 | 0.00 | 0.81 | -16.19 | 296.48 | -29.80 | 111.71 | 0.5158 | -784.0 | -658.1 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -16.78 | 295.87 | -30.41 | 112.48 | 0.5266 | -709.0 | -619.4 | |
| 0.00 | 1.50 | 0.00 | 0.87 | -14.12 | 295.87 | -30.41 | 107.51 | 0.5168 | -788.0 | -629.4 | |
| 0.00 | 2.64 | 0.00 | 1.52 | -11.85 | 296.11 | -30.17 | 103.22 | 0.5073 | -865.0 | -734.4 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -12.05 | 295.84 | -30.44 | 103.53 | 0.5117 | -644.0 | -497.2 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -13.84 | 294.14 | -32.14 | 106.37 | 0.5405 | -668.0 | -490.6 | |
| 0.00 | 1.32 | 0.00 | 0.79 | -15.61 | 293.13 | -33.15 | 109.18 | 0.5597 | -607.0 | -489.1 | |
| 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. | |