SDO HMI 2011-05-28 13:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.43 | 36.54 | 7.93 | 18.80 | -15.92 | 113.41 | 4.46 | 196.02 | 0.2693 | -599.3 | -417.2 | |
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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 |
| 0.72 | 2.26 | 0.37 | 1.17 | -15.65 | 118.57 | 9.63 | 212.68 | 0.2995 | 987.5 | 845.8 | |
| 0.00 | 1.35 | 0.00 | 0.70 | -15.43 | 118.56 | 9.62 | 213.07 | 0.2964 | 833.0 | 692.9 | |
| 0.00 | 1.35 | 0.00 | 0.70 | -15.65 | 118.22 | 9.27 | 211.73 | 0.2964 | 889.0 | 696.2 | |
| 0.00 | 2.89 | 0.00 | 1.49 | -16.07 | 113.66 | 4.71 | 197.01 | 0.2708 | -651.0 | -564.0 | |
| 0.00 | 1.08 | 0.00 | 0.56 | -15.97 | 113.50 | 4.55 | 196.56 | 0.2685 | -997.0 | -747.1 | |
| 0.00 | 1.44 | 0.00 | 0.75 | -17.45 | 113.47 | 4.52 | 194.97 | 0.2923 | -840.0 | -648.9 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -15.94 | 113.34 | 4.39 | 196.05 | 0.2673 | -876.0 | -580.7 | |
| 0.00 | 2.80 | 0.00 | 1.44 | -15.85 | 112.89 | 3.94 | 194.59 | 0.2638 | -799.0 | -861.9 | |
| 2.62 | 11.73 | 1.35 | 6.03 | -16.41 | 112.65 | 3.70 | 193.21 | 0.2721 | -832.6 | -774.6 | |
| 5.86 | 7.22 | 3.01 | 3.70 | -15.85 | 112.57 | 3.63 | 193.46 | 0.2625 | -1128.0 | -824.8 | |
| 6.23 | -9.00 | 3.20 | -9.00 | -16.22 | 112.49 | 3.54 | 192.81 | 0.2683 | -1080.7 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.68 | -12.57 | 111.09 | 2.14 | 190.41 | 0.2027 | -887.0 | -675.8 | |
| 0.00 | 2.26 | 0.00 | 1.16 | -15.85 | 111.03 | 2.08 | 187.81 | 0.2577 | -792.0 | -671.4 | |
| 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. | |