SDO HMI 2011-08-28 13:59:08 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.41 | 39.63 | 4.75 | 20.03 | 16.93 | 328.43 | -3.41 | 324.86 | 0.1915 | 251.5 | -57.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.23 | 0.00 | 1.61 | 13.49 | 334.69 | 2.85 | 336.52 | 0.1219 | -860.0 | -689.9 | |
| 0.00 | 2.87 | 0.00 | 1.43 | 12.73 | 334.34 | 2.50 | 336.55 | 0.1074 | -856.0 | -726.5 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 17.72 | 332.42 | 0.59 | 356.96 | 0.1853 | -909.0 | -789.6 | |
| 0.00 | 1.26 | 0.00 | 0.63 | 17.72 | 332.17 | 0.33 | 358.27 | 0.1851 | -900.0 | -686.4 | |
| 1.61 | 5.02 | 0.82 | 2.55 | 19.44 | 329.19 | -2.65 | 11.52 | 0.2192 | -996.6 | -741.3 | |
| 0.00 | 1.61 | 0.00 | 0.82 | 19.16 | 328.65 | -3.19 | 14.12 | 0.2165 | -849.0 | -805.8 | |
| 4.84 | 11.92 | 2.44 | 6.01 | 17.25 | 328.62 | -3.22 | 16.92 | 0.1851 | 983.2 | 732.8 | |
| 2.96 | -7.00 | 1.49 | -7.00 | 17.15 | 328.37 | -3.47 | 18.32 | 0.1848 | 1027.6 | 999999 | |
| 0.00 | 1.70 | 0.00 | 0.87 | 19.21 | 327.26 | -4.57 | 19.72 | 0.2242 | -857.0 | -698.6 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 15.88 | 326.37 | -5.47 | 30.92 | 0.1792 | 959.0 | 786.5 | |
| 0.00 | 2.42 | 0.00 | 1.24 | 20.91 | 326.11 | -5.73 | 21.30 | 0.2578 | 782.0 | 546.9 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 15.44 | 325.53 | -6.31 | 36.03 | 0.1809 | 770.0 | 459.9 | |
| 0.00 | 0.90 | 0.00 | 0.45 | 13.82 | 323.72 | -8.12 | 49.24 | 0.1818 | 800.0 | 624.9 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 13.48 | 323.51 | -8.32 | 51.41 | 0.1809 | 932.0 | 675.1 | |
| 0.00 | 1.17 | 0.00 | 0.59 | 14.37 | 321.93 | -9.91 | 52.44 | 0.2112 | 854.0 | 630.2 | |
| 0.00 | 1.08 | 0.00 | 0.56 | 18.45 | 319.40 | -12.43 | 45.66 | 0.2868 | 920.0 | 696.0 | |
| 0.00 | 0.99 | 0.00 | 0.51 | 16.57 | 319.24 | -12.59 | 51.32 | 0.2689 | 816.0 | 606.5 | |
| 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. | |