SDO HMI 2014-04-22 07:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 69.98 | 412.11 | 37.70 | 222.08 | 17.80 | 166.71 | 3.84 | 350.67 | 0.3952 | -666.7 | -337.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.39 | 379.61 | 5.61 | 204.57 | 18.01 | 167.54 | 4.67 | 348.80 | 0.4000 | -1074.8 | -421.5 | |
| 52.58 | -1.00 | 28.32 | -1.00 | 17.74 | 167.06 | 4.18 | 349.81 | 0.3944 | -1386.5 | 999999 | |
| 0.00 | 1.42 | 0.00 | 0.77 | 18.69 | 163.80 | 0.93 | 357.82 | 0.4039 | 633.0 | 433.3 | |
| 0.00 | 4.44 | 0.00 | 2.38 | 17.51 | 163.73 | 0.86 | 357.87 | 0.3848 | 859.0 | 768.0 | |
| 0.00 | 1.87 | 0.00 | 1.00 | 17.41 | 163.41 | 0.54 | 358.65 | 0.3831 | 942.0 | 788.5 | |
| 0.80 | 2.66 | 0.43 | 1.43 | 17.83 | 163.35 | 0.48 | 358.83 | 0.3899 | 874.1 | 746.1 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 17.67 | 163.19 | 0.32 | 359.21 | 0.3872 | 843.0 | 695.7 | |
| 0.00 | 2.40 | 0.00 | 1.31 | 19.88 | 162.72 | -0.16 | 0.35 | 0.4226 | 589.0 | 566.7 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 18.00 | 162.31 | -0.57 | 1.38 | 0.3926 | 734.0 | 623.7 | |
| 0.00 | 1.51 | 0.00 | 0.81 | 18.33 | 162.21 | -0.66 | 1.59 | 0.3979 | 897.0 | 740.6 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 17.41 | 161.30 | -1.58 | 3.94 | 0.3839 | 902.0 | 775.0 | |
| 0.00 | 1.24 | 0.00 | 0.67 | 17.22 | 161.24 | -1.64 | 4.13 | 0.3808 | 1061.0 | 902.1 | |
| 1.15 | 2.49 | 0.62 | 1.34 | 17.91 | 160.37 | -2.50 | 6.09 | 0.3932 | 859.3 | 607.6 | |
| 5.06 | 9.41 | 2.72 | 5.05 | 17.38 | 160.25 | -2.62 | 6.53 | 0.3850 | 1127.7 | 806.5 | |
| 0.00 | 1.78 | 0.00 | 0.98 | 20.73 | 158.59 | -4.28 | 9.14 | 0.4415 | 517.0 | 473.9 | |
| 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. | |