SDO HMI 2011-05-26 04:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.10 | 61.93 | 12.05 | 35.22 | -15.68 | 114.36 | -25.99 | 120.58 | 0.4919 | 217.6 | 178.9 | |
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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 |
| 0.00 | 1.08 | 0.00 | 0.60 | -15.23 | 116.39 | -23.96 | 121.59 | 0.4618 | 1022.0 | 836.2 | |
| 0.00 | 1.98 | 0.00 | 1.11 | -15.57 | 116.25 | -24.10 | 122.10 | 0.4663 | 959.0 | 780.5 | |
| 0.81 | 16.41 | 0.46 | 9.22 | -16.23 | 116.13 | -24.22 | 123.21 | 0.4727 | 922.3 | 739.3 | |
| 4.15 | -3.00 | 2.33 | -3.00 | -15.98 | 116.02 | -24.33 | 122.64 | 0.4722 | 984.9 | 999999 | |
| 0.00 | 1.71 | 0.00 | 0.97 | -16.51 | 115.85 | -24.50 | 123.45 | 0.4785 | 770.0 | 572.4 | |
| 3.07 | -3.00 | 1.72 | -3.00 | -15.79 | 115.91 | -24.44 | 122.17 | 0.4723 | 851.8 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -16.38 | 115.03 | -25.32 | 122.41 | 0.4880 | 742.0 | 565.5 | |
| 0.00 | 2.80 | 0.00 | 1.59 | -16.47 | 114.77 | -25.58 | 122.34 | 0.4921 | 164.0 | 316.7 | |
| 0.00 | 1.80 | 0.00 | 1.02 | -14.75 | 115.00 | -25.35 | 119.37 | 0.4770 | 876.0 | 708.6 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -14.93 | 114.83 | -25.51 | 119.57 | 0.4805 | 644.0 | 439.9 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -14.65 | 114.80 | -25.55 | 119.01 | 0.4790 | 672.0 | 508.0 | |
| 0.00 | 5.59 | 0.00 | 3.18 | -14.73 | 113.81 | -26.54 | 118.33 | 0.4929 | 684.0 | 521.5 | |
| 2.07 | 11.54 | 1.19 | 6.60 | -15.32 | 113.41 | -26.94 | 119.09 | 0.5019 | -947.1 | -616.5 | |
| 5.59 | 9.11 | 3.23 | 5.26 | -16.23 | 112.75 | -27.60 | 120.16 | 0.5165 | -878.3 | -621.4 | |
| 5.41 | 6.58 | 3.12 | 3.79 | -15.60 | 112.81 | -27.54 | 119.10 | 0.5117 | -922.4 | -717.1 | |
| 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. | |