SDO HMI 2014-04-22 00:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.07 | 413.53 | 36.62 | 222.38 | 17.75 | 166.86 | 0.14 | 359.67 | 0.3901 | -777.1 | -350.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.65 | 387.69 | 5.74 | 208.45 | 18.04 | 167.64 | 0.92 | 357.76 | 0.3942 | -1063.0 | -409.3 | |
| 51.48 | -1.00 | 27.66 | -1.00 | 17.71 | 167.14 | 0.42 | 358.98 | 0.3887 | -1274.6 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 18.57 | 165.71 | -1.01 | 2.39 | 0.4028 | -497.0 | -439.0 | |
| 0.00 | 3.11 | 0.00 | 1.67 | 17.56 | 163.69 | -3.03 | 7.47 | 0.3894 | 904.0 | 757.9 | |
| 0.00 | 1.07 | 0.00 | 0.57 | 17.14 | 163.57 | -3.15 | 7.92 | 0.3829 | 792.0 | 677.8 | |
| 0.00 | 1.42 | 0.00 | 0.76 | 17.33 | 163.31 | -3.41 | 8.47 | 0.3866 | 763.0 | 589.0 | |
| 0.00 | 1.33 | 0.00 | 0.73 | 19.18 | 162.13 | -4.59 | 10.44 | 0.4189 | 888.0 | 657.5 | |
| 0.00 | 1.15 | 0.00 | 0.62 | 17.48 | 161.60 | -5.12 | 12.53 | 0.3939 | 850.0 | 642.2 | |
| 2.04 | 3.82 | 1.11 | 2.07 | 17.95 | 160.41 | -6.31 | 15.00 | 0.4058 | 764.0 | 552.5 | |
| 2.66 | 10.21 | 1.44 | 5.51 | 17.56 | 160.33 | -6.39 | 15.45 | 0.4001 | 1007.9 | 848.2 | |
| 0.00 | 0.89 | 0.00 | 0.48 | 18.64 | 160.16 | -6.56 | 15.09 | 0.4174 | -674.0 | -535.8 | |
| 1.24 | -10.00 | 0.67 | -10.00 | 17.40 | 160.11 | -6.61 | 16.07 | 0.3985 | 875.2 | 999999 | |
| 0.00 | 1.95 | 0.00 | 1.04 | 14.81 | 160.10 | -6.62 | 18.19 | 0.3587 | 773.0 | 610.4 | |
| 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. | |