SDO HMI 2011-06-04 00:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.66 | 149.02 | 15.71 | 79.11 | -20.89 | 18.79 | -4.66 | 167.92 | 0.3608 | 807.0 | 437.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.72 | -21.23 | 20.91 | -2.55 | 173.36 | 0.3602 | -756.0 | -672.9 | |
| 28.21 | 121.88 | 14.94 | 64.53 | -20.64 | 19.22 | -4.23 | 168.73 | 0.3550 | 1297.8 | 449.3 | |
| 0.00 | 1.45 | 0.00 | 0.77 | -20.97 | 18.63 | -4.83 | 167.41 | 0.3622 | 836.0 | 663.9 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -22.34 | 18.48 | -4.98 | 167.90 | 0.3844 | 839.0 | 635.5 | |
| 1.45 | 1.45 | 0.77 | 0.77 | -21.19 | 18.49 | -4.97 | 167.21 | 0.3663 | 755.5 | 752.0 | |
| 0.00 | 1.09 | 0.00 | 0.58 | -21.16 | 18.10 | -5.36 | 166.22 | 0.3673 | 897.0 | 718.7 | |
| 0.00 | 4.25 | 0.00 | 2.27 | -21.75 | 18.07 | -5.38 | 166.57 | 0.3766 | 818.0 | 786.8 | |
| 0.00 | 1.72 | 0.00 | 0.92 | -21.39 | 17.99 | -5.47 | 166.12 | 0.3713 | 992.0 | 749.2 | |
| 0.00 | 4.52 | 0.00 | 2.42 | -21.68 | 17.81 | -5.64 | 165.90 | 0.3766 | 839.0 | 766.2 | |
| 0.00 | 4.70 | 0.00 | 2.51 | -21.72 | 17.52 | -5.94 | 165.21 | 0.3783 | 762.0 | 763.4 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -22.50 | 12.69 | -10.77 | 155.40 | 0.4163 | -833.0 | -696.3 | |
| 0.00 | 2.62 | 0.00 | 1.44 | -23.39 | 12.08 | -11.38 | 155.17 | 0.4330 | -670.0 | -555.7 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -23.69 | 11.68 | -11.78 | 154.74 | 0.4398 | -705.0 | -627.6 | |
| 0.00 | 0.81 | 0.00 | 0.46 | -25.05 | 9.79 | -13.66 | 152.88 | 0.4714 | -629.0 | -476.6 | |
| 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. | |