SDO HMI 2011-05-04 05:59:07 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.14 | 317.37 | 29.20 | 171.50 | 17.81 | 61.45 | -9.30 | 22.57 | 0.4014 | -747.9 | -361.6 | |
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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 |
| 46.10 | 297.53 | 24.85 | 160.42 | 17.61 | 61.84 | -8.91 | 22.00 | 0.3959 | -1367.9 | -429.9 | |
| 0.00 | 1.70 | 0.00 | 0.96 | 23.05 | 61.45 | -9.30 | 18.21 | 0.4779 | -718.0 | -605.4 | |
| 6.97 | -1.00 | 3.77 | -1.00 | 18.00 | 61.37 | -9.38 | 22.64 | 0.4046 | -882.9 | 999999 | |
| 1.07 | -1.00 | 0.58 | -1.00 | 17.98 | 61.08 | -9.67 | 23.29 | 0.4060 | -700.8 | 999999 | |
| 0.00 | 1.97 | 0.00 | 1.07 | 18.49 | 59.24 | -11.52 | 26.54 | 0.4257 | -743.0 | -617.4 | |
| 0.00 | 1.88 | 0.00 | 1.05 | 20.13 | 57.57 | -13.19 | 27.87 | 0.4602 | 738.0 | 611.6 | |
| 0.00 | 1.34 | 0.00 | 0.74 | 18.42 | 57.22 | -13.54 | 30.46 | 0.4400 | 838.0 | 689.4 | |
| 0.00 | 2.77 | 0.00 | 1.53 | 18.52 | 56.95 | -13.81 | 30.83 | 0.4435 | 1056.0 | 828.2 | |
| 0.00 | 0.89 | 0.00 | 0.49 | 17.45 | 57.03 | -13.72 | 32.02 | 0.4286 | 836.0 | 691.3 | |
| 0.00 | 1.70 | 0.00 | 0.94 | 18.72 | 56.93 | -13.83 | 30.62 | 0.4462 | 971.0 | 780.8 | |
| 0.00 | 1.52 | 0.00 | 0.84 | 18.40 | 56.33 | -14.42 | 32.07 | 0.4469 | 825.0 | 654.1 | |
| 0.00 | 2.14 | 0.00 | 1.19 | 18.28 | 56.24 | -14.51 | 32.39 | 0.4460 | 905.0 | 737.7 | |
| 0.00 | 1.52 | 0.00 | 0.89 | 25.17 | 55.37 | -15.38 | 26.42 | 0.5418 | 862.0 | 658.4 | |
| 0.00 | 1.25 | 0.00 | 0.70 | 19.59 | 54.56 | -16.19 | 33.59 | 0.4769 | 620.0 | 427.2 | |
| 0.00 | 1.16 | 0.00 | 0.68 | 22.43 | 52.42 | -18.33 | 33.45 | 0.5295 | 726.0 | 586.5 | |
| 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. | |