SDO HMI 2011-06-30 12:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.36 | 28.16 | 1.20 | 14.42 | 14.91 | 24.71 | -8.02 | 32.83 | 0.2520 | -415.0 | -304.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.09 | 0.00 | 0.56 | 18.59 | 27.00 | -5.73 | 19.12 | 0.2900 | -885.0 | -679.8 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 15.50 | 26.11 | -6.62 | 26.71 | 0.2482 | -783.0 | -573.8 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 15.62 | 25.56 | -7.16 | 28.32 | 0.2543 | -908.0 | -724.4 | |
| 2.36 | 5.36 | 1.20 | 2.72 | 13.10 | 25.52 | -7.21 | 34.21 | 0.2183 | 1021.3 | 596.3 | |
| 0.00 | 1.73 | 0.00 | 0.88 | 15.69 | 25.40 | -7.32 | 28.73 | 0.2565 | -915.0 | -726.9 | |
| 0.00 | 1.09 | 0.00 | 0.55 | 10.17 | 25.31 | -7.41 | 44.50 | 0.1820 | -801.0 | -716.5 | |
| 0.00 | 2.45 | 0.00 | 1.26 | 15.56 | 25.05 | -7.67 | 30.11 | 0.2575 | -714.0 | -634.3 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 13.97 | 24.89 | -7.84 | 34.21 | 0.2364 | -823.0 | -585.9 | |
| 0.00 | 2.45 | 0.00 | 1.25 | 13.50 | 24.46 | -8.26 | 36.82 | 0.2342 | 121.0 | 100.3 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 15.71 | 24.31 | -8.41 | 32.11 | 0.2661 | -971.0 | -753.5 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 16.11 | 24.07 | -8.65 | 32.00 | 0.2740 | -815.0 | -721.3 | |
| 0.00 | 1.91 | 0.00 | 0.98 | 14.05 | 23.84 | -8.89 | 37.37 | 0.2480 | 812.0 | 564.1 | |
| 0.00 | 1.82 | 0.00 | 0.94 | 16.24 | 23.65 | -9.08 | 32.97 | 0.2795 | -831.0 | -649.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 17.43 | 23.14 | -9.59 | 32.06 | 0.3007 | -776.0 | -559.3 | |
| 0.00 | 1.09 | 0.00 | 0.57 | 17.19 | 21.10 | -11.62 | 37.59 | 0.3169 | 755.0 | 620.5 | |
| 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. | |