SDO HMI 2014-04-04 10:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 50.46 | 214.45 | 27.71 | 117.41 | 17.01 | 29.57 | -9.30 | 21.18 | 0.4273 | -7.9 | -240.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.79 | 155.62 | 9.16 | 84.75 | 17.12 | 31.13 | -7.75 | 17.96 | 0.4195 | -1120.3 | -443.5 | |
| 1.41 | -1.00 | 0.76 | -1.00 | 16.54 | 30.93 | -7.94 | 18.86 | 0.4117 | -1316.1 | 999999 | |
| 9.76 | -1.00 | 5.31 | -1.00 | 16.74 | 30.76 | -8.11 | 19.06 | 0.4155 | -1114.8 | 999999 | |
| 0.00 | 2.73 | 0.00 | 1.48 | 15.89 | 29.09 | -9.78 | 23.43 | 0.4126 | -952.0 | -777.5 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 15.97 | 28.77 | -10.10 | 24.04 | 0.4157 | -593.0 | -460.3 | |
| 0.00 | 1.23 | 0.00 | 0.68 | 17.18 | 27.02 | -11.86 | 26.32 | 0.4447 | 833.0 | 693.8 | |
| 0.00 | 2.55 | 0.00 | 1.41 | 16.55 | 26.25 | -12.62 | 28.45 | 0.4414 | 843.0 | 698.3 | |
| 0.70 | 41.32 | 0.39 | 22.94 | 17.24 | 26.02 | -12.86 | 28.14 | 0.4526 | 739.1 | 613.3 | |
| 12.13 | -8.00 | 6.72 | -8.00 | 17.01 | 25.93 | -12.94 | 28.54 | 0.4501 | 1110.3 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.64 | 17.64 | 25.83 | -13.05 | 28.05 | 0.4594 | 29.0 | 50.2 | |
| 9.67 | -8.00 | 5.37 | -8.00 | 17.18 | 25.57 | -13.31 | 29.02 | 0.4552 | 986.4 | 999999 | |
| 0.00 | 3.96 | 0.00 | 2.21 | 17.43 | 25.06 | -13.81 | 29.65 | 0.4623 | 796.0 | 647.7 | |
| 0.00 | 0.97 | 0.00 | 0.55 | 18.56 | 24.65 | -14.23 | 29.14 | 0.4805 | 646.0 | 535.8 | |
| 0.00 | 1.76 | 0.00 | 0.99 | 18.23 | 24.58 | -14.30 | 29.61 | 0.4767 | 728.0 | 527.5 | |
| 0.00 | 1.85 | 0.00 | 1.04 | 18.37 | 24.37 | -14.50 | 29.81 | 0.4800 | 767.0 | 564.1 | |
| 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. | |