SDO HMI 2011-07-01 01:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.16 | 54.94 | 6.15 | 27.86 | 14.83 | 25.03 | -0.50 | 1.73 | 0.2105 | -75.3 | -235.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.36 | 0.00 | 0.70 | 16.24 | 30.02 | 4.49 | 342.04 | 0.2450 | -800.0 | -610.1 | |
| 9.08 | 18.89 | 4.58 | 9.52 | 13.19 | 26.41 | 0.89 | 355.20 | 0.1813 | 1083.2 | 837.3 | |
| 0.00 | 4.72 | 0.00 | 2.40 | 15.40 | 25.13 | -0.40 | 1.76 | 0.2187 | -851.0 | -647.3 | |
| 0.00 | 1.00 | 0.00 | 0.51 | 15.78 | 24.90 | -0.62 | 2.66 | 0.2253 | -929.0 | -757.9 | |
| 0.00 | 5.00 | 0.00 | 2.55 | 16.37 | 24.62 | -0.91 | 3.72 | 0.2357 | -978.0 | -807.6 | |
| 2.09 | 4.36 | 1.06 | 2.20 | 14.34 | 24.53 | -0.99 | 4.81 | 0.2011 | -970.4 | -736.5 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 14.06 | 24.44 | -1.09 | 5.40 | 0.1965 | -944.0 | -643.4 | |
| 0.00 | 4.27 | 0.00 | 2.17 | 15.84 | 24.30 | -1.22 | 5.21 | 0.2270 | -786.0 | -639.5 | |
| 0.00 | 2.18 | 0.00 | 1.10 | 13.41 | 24.22 | -1.30 | 6.87 | 0.1857 | 902.0 | 641.6 | |
| 0.45 | 5.36 | 0.23 | 2.72 | 15.28 | 23.96 | -1.57 | 6.98 | 0.2181 | -1003.6 | -875.4 | |
| 0.00 | 1.63 | 0.00 | 0.84 | 17.25 | 23.17 | -2.35 | 8.93 | 0.2532 | -839.0 | -753.7 | |
| 0.00 | 2.27 | 0.00 | 1.16 | 17.37 | 22.76 | -2.77 | 10.39 | 0.2565 | -830.0 | -594.3 | |
| 0.54 | 1.36 | 0.28 | 0.70 | 18.00 | 21.62 | -3.90 | 13.88 | 0.2708 | 780.3 | 612.4 | |
| 0.00 | 1.09 | 0.00 | 0.56 | 17.56 | 20.77 | -4.75 | 17.26 | 0.2675 | 991.0 | 716.2 | |
| 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. | |