SDO HMI 2011-06-02 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 |
| 26.93 | 169.08 | 16.47 | 103.08 | -20.53 | 19.39 | -30.53 | 125.74 | 0.5881 | 638.1 | 460.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.85 | -20.21 | 23.34 | -26.58 | 128.73 | 0.5403 | -505.0 | -512.0 | |
| 0.00 | 2.71 | 0.00 | 1.60 | -19.40 | 22.26 | -27.66 | 126.45 | 0.5465 | -815.0 | -662.7 | |
| 0.00 | 1.17 | 0.00 | 0.69 | -19.05 | 22.25 | -27.67 | 125.88 | 0.5439 | -734.0 | -569.2 | |
| 0.00 | 1.36 | 0.00 | 0.80 | -18.47 | 22.06 | -27.86 | 124.80 | 0.5418 | -765.0 | -636.8 | |
| 1.27 | 2.17 | 0.75 | 1.28 | -18.79 | 21.64 | -28.28 | 124.94 | 0.5493 | -764.6 | -516.7 | |
| 17.53 | 149.74 | 10.70 | 91.31 | -20.42 | 19.57 | -30.35 | 125.71 | 0.5854 | 1211.2 | 518.3 | |
| 0.54 | -6.00 | 0.33 | -6.00 | -20.68 | 19.14 | -30.79 | 125.75 | 0.5922 | 736.3 | 999999 | |
| 6.42 | -6.00 | 3.96 | -6.00 | -20.81 | 18.77 | -31.16 | 125.65 | 0.5974 | 703.5 | 999999 | |
| 1.17 | 4.07 | 0.73 | 2.52 | -21.33 | 18.61 | -31.32 | 126.27 | 0.6028 | 665.6 | 518.8 | |
| 0.00 | 2.98 | 0.00 | 1.85 | -21.07 | 18.36 | -31.56 | 125.71 | 0.6037 | 637.0 | 504.8 | |
| 0.00 | 0.99 | 0.00 | 0.62 | -21.16 | 17.45 | -32.47 | 125.16 | 0.6147 | 731.0 | 534.9 | |
| 0.00 | 0.81 | 0.00 | 0.52 | -22.66 | 16.35 | -33.57 | 126.47 | 0.6368 | 602.0 | 585.1 | |
| 0.00 | 1.36 | 0.00 | 0.87 | -22.30 | 16.30 | -33.63 | 125.93 | 0.6350 | 702.0 | 554.3 | |
| 0.00 | 0.27 | 0.00 | 0.17 | -22.59 | 16.21 | -33.71 | 126.28 | 0.6379 | 400.0 | 331.3 | |
| 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. | |