SDO HMI 2011-05-02 06:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.05 | 18.02 | 1.15 | 9.83 | 14.18 | 113.39 | 16.75 | 318.07 | 0.4201 | -780.7 | -681.2 | |
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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 |
| 2.05 | 2.59 | 1.15 | 1.44 | 14.06 | 117.34 | 20.70 | 311.83 | 0.4620 | -835.0 | -749.2 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 10.12 | 114.29 | 17.65 | 309.03 | 0.3859 | -756.0 | -530.0 | |
| 0.00 | 1.34 | 0.00 | 0.73 | 14.90 | 113.68 | 17.04 | 318.68 | 0.4307 | -684.0 | -578.7 | |
| 0.00 | 0.80 | 0.00 | 0.44 | 14.67 | 113.60 | 16.96 | 318.46 | 0.4272 | -712.0 | -630.1 | |
| 0.00 | 1.43 | 0.00 | 0.78 | 14.34 | 112.92 | 16.28 | 319.06 | 0.4163 | -836.0 | -708.8 | |
| 0.00 | 1.87 | 0.00 | 1.02 | 14.91 | 112.74 | 16.10 | 320.30 | 0.4211 | -753.0 | -591.3 | |
| 0.00 | 0.98 | 0.00 | 0.53 | 13.70 | 112.58 | 15.94 | 318.59 | 0.4051 | -792.0 | -734.4 | |
| 0.00 | 0.80 | 0.00 | 0.43 | 13.54 | 112.51 | 15.87 | 318.46 | 0.4025 | -733.0 | -613.1 | |
| 0.00 | 1.61 | 0.00 | 0.88 | 15.96 | 112.53 | 15.89 | 322.26 | 0.4318 | -808.0 | -672.2 | |
| 0.00 | 1.16 | 0.00 | 0.64 | 15.74 | 112.51 | 15.87 | 321.96 | 0.4289 | -799.0 | -701.1 | |
| 0.00 | 4.46 | 0.00 | 2.41 | 13.65 | 112.03 | 15.39 | 319.51 | 0.3988 | -871.0 | -774.3 | |
| 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. | |