SDO HMI 2011-06-03 07:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.85 | 35.65 | 6.32 | 18.80 | 17.39 | 41.47 | 8.62 | 336.02 | 0.3435 | -30.8 | 158.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.22 | 13.65 | 5.47 | 7.31 | 18.11 | 45.51 | 12.66 | 326.75 | 0.3816 | -986.4 | -819.6 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 21.52 | 45.19 | 12.34 | 331.97 | 0.4250 | 756.0 | 609.7 | |
| 0.00 | 1.72 | 0.00 | 0.90 | 16.13 | 42.89 | 10.04 | 329.55 | 0.3319 | -981.0 | -711.0 | |
| 1.63 | 3.35 | 0.85 | 1.76 | 16.92 | 41.51 | 8.67 | 334.20 | 0.3326 | -952.5 | -681.2 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.64 | 41.43 | 8.59 | 334.00 | 0.3278 | -898.0 | -696.8 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 16.29 | 41.00 | 8.16 | 334.66 | 0.3195 | -755.0 | -698.7 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 15.90 | 38.47 | 5.62 | 341.47 | 0.2978 | 831.0 | 624.2 | |
| 0.00 | 0.90 | 0.00 | 0.47 | 16.70 | 38.24 | 5.39 | 343.00 | 0.3092 | 972.0 | 724.2 | |
| 0.00 | 1.45 | 0.00 | 0.75 | 16.73 | 37.35 | 4.50 | 345.71 | 0.3057 | 885.0 | 658.2 | |
| 0.00 | 2.08 | 0.00 | 1.08 | 16.48 | 37.15 | 4.30 | 346.10 | 0.3008 | 1005.0 | 847.9 | |
| 0.00 | 1.18 | 0.00 | 0.61 | 16.44 | 36.86 | 4.02 | 346.96 | 0.2992 | 949.0 | 705.5 | |
| 0.00 | 3.98 | 0.00 | 2.07 | 16.70 | 35.82 | 2.97 | 350.42 | 0.2999 | 834.0 | 674.1 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 16.25 | 35.69 | 2.84 | 350.59 | 0.2922 | 1035.0 | 875.8 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 17.40 | 35.13 | 2.28 | 352.92 | 0.3098 | 1008.0 | 788.3 | |
| 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. | |