SDO HMI 2011-05-27 05:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.96 | 112.41 | 28.35 | 60.20 | 20.60 | 130.37 | 3.80 | 350.70 | 0.3805 | -67.8 | 16.4 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.19 | 51.97 | 12.48 | 27.96 | 21.02 | 132.34 | 5.77 | 346.11 | 0.3925 | -1093.5 | -541.9 | |
| 3.97 | -1.00 | 2.13 | -1.00 | 20.72 | 131.80 | 5.24 | 347.16 | 0.3858 | -1105.5 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.68 | 20.43 | 131.53 | 4.97 | 347.63 | 0.3802 | -911.0 | -660.3 | |
| 0.00 | 3.52 | 0.00 | 1.89 | 21.38 | 130.68 | 4.11 | 350.16 | 0.3926 | -878.0 | -716.2 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 19.97 | 130.13 | 3.56 | 350.86 | 0.3686 | 858.0 | 666.1 | |
| 0.00 | 1.44 | 0.00 | 0.78 | 21.38 | 130.03 | 3.46 | 351.70 | 0.3909 | -548.0 | -417.4 | |
| 0.00 | 1.08 | 0.00 | 0.57 | 19.54 | 129.76 | 3.19 | 351.60 | 0.3609 | 718.0 | 473.6 | |
| 0.00 | 3.25 | 0.00 | 1.74 | 20.62 | 129.49 | 2.92 | 352.71 | 0.3776 | 748.0 | 623.9 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 21.28 | 129.24 | 2.67 | 353.54 | 0.3877 | -821.0 | -638.8 | |
| 2.53 | 7.58 | 1.35 | 4.05 | 20.62 | 129.17 | 2.60 | 353.51 | 0.3770 | 694.5 | 651.9 | |
| 1.89 | -10.00 | 1.01 | -10.00 | 20.46 | 128.94 | 2.37 | 354.04 | 0.3739 | 854.1 | 999999 | |
| 0.00 | 2.89 | 0.00 | 1.53 | 19.80 | 128.89 | 2.32 | 353.94 | 0.3633 | 594.0 | 563.2 | |
| 3.34 | 4.15 | 1.77 | 2.20 | 19.48 | 128.76 | 2.19 | 354.19 | 0.3578 | 1065.0 | 759.4 | |
| 18.04 | 32.75 | 9.61 | 17.45 | 20.16 | 128.06 | 1.49 | 356.18 | 0.3679 | 1050.1 | 778.0 | |
| 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. | |