SDO HMI 2014-05-31 01:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.01 | 97.34 | 13.48 | 50.30 | -9.10 | 24.75 | 14.26 | 238.79 | 0.2855 | 598.6 | 525.0 | |
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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 | 0.90 | 0.00 | 0.47 | -6.87 | 27.06 | 16.57 | 249.46 | 0.3037 | 751.0 | 609.9 | |
| 1.81 | 15.08 | 0.94 | 7.85 | -9.04 | 26.44 | 15.95 | 242.10 | 0.3085 | 889.8 | 798.6 | |
| 3.43 | -2.00 | 1.78 | -2.00 | -8.77 | 26.40 | 15.91 | 242.85 | 0.3058 | 1054.0 | 999999 | |
| 3.97 | 59.70 | 2.06 | 30.91 | -9.26 | 25.46 | 14.97 | 239.97 | 0.2958 | 869.7 | 600.0 | |
| 15.99 | -4.00 | 8.28 | -4.00 | -8.95 | 25.42 | 14.93 | 240.82 | 0.2927 | 1208.5 | 999999 | |
| 0.00 | 6.41 | 0.00 | 3.30 | -9.82 | 23.51 | 13.03 | 234.76 | 0.2731 | 906.0 | 707.4 | |
| 0.00 | 1.54 | 0.00 | 0.79 | -9.82 | 23.23 | 12.74 | 234.17 | 0.2692 | 943.0 | 848.8 | |
| 0.00 | 2.26 | 0.00 | 1.16 | -10.22 | 23.18 | 12.69 | 232.86 | 0.2725 | 925.0 | 752.4 | |
| 0.81 | 3.70 | 0.42 | 1.90 | -10.06 | 22.95 | 12.47 | 232.83 | 0.2679 | 1084.9 | 766.0 | |
| 0.00 | 1.99 | 0.00 | 1.01 | -8.50 | 20.52 | 10.03 | 232.11 | 0.2192 | -897.0 | -697.7 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -4.47 | 20.10 | 9.61 | 248.97 | 0.1792 | -767.0 | -566.4 | |
| 0.00 | 1.26 | 0.00 | 0.64 | -8.69 | 20.02 | 9.54 | 230.05 | 0.2146 | -853.0 | -664.1 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -10.47 | 17.14 | 6.65 | 214.15 | 0.2038 | -813.0 | -564.6 | |
| 0.00 | 0.99 | 0.00 | 0.50 | -10.22 | 17.04 | 6.55 | 214.46 | 0.1994 | -857.0 | -594.9 | |
| 0.00 | 1.17 | 0.00 | 0.59 | -11.99 | 14.08 | 3.60 | 197.57 | 0.2042 | -734.0 | -508.2 | |
| 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. | |