SDO HMI 2014-05-31 14:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.86 | 59.06 | 11.81 | 31.74 | -8.80 | 24.69 | 21.34 | 248.51 | 0.3882 | 532.1 | 328.6 | |
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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 |
| 2.17 | 7.95 | 1.18 | 4.32 | -8.58 | 26.60 | 23.25 | 250.60 | 0.4156 | 925.5 | 760.1 | |
| 0.00 | 1.63 | 0.00 | 0.89 | -8.86 | 26.62 | 23.27 | 249.98 | 0.4172 | 875.0 | 789.1 | |
| 0.00 | 1.35 | 0.00 | 0.74 | -11.02 | 26.01 | 22.66 | 244.62 | 0.4202 | 765.0 | 605.4 | |
| 19.69 | 35.13 | 10.63 | 18.96 | -8.86 | 25.42 | 22.07 | 249.04 | 0.3992 | 1064.8 | 660.1 | |
| 0.00 | 1.17 | 0.00 | 0.63 | -10.13 | 23.45 | 20.10 | 244.15 | 0.3775 | 776.0 | 647.8 | |
| 0.00 | 0.54 | 0.00 | 0.29 | -10.23 | 23.10 | 19.74 | 243.53 | 0.3730 | 878.0 | 632.2 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -9.95 | 22.36 | 19.01 | 243.39 | 0.3603 | 762.0 | 578.4 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -4.33 | 20.71 | 17.36 | 258.03 | 0.3055 | -758.0 | -534.2 | |
| 0.00 | 3.34 | 0.00 | 1.75 | -9.19 | 20.66 | 17.31 | 243.35 | 0.3301 | -862.0 | -755.9 | |
| 0.00 | 1.99 | 0.00 | 1.04 | -8.76 | 20.48 | 17.13 | 244.32 | 0.3244 | -1013.0 | -862.0 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -8.97 | 20.43 | 17.07 | 243.64 | 0.3251 | -803.0 | -777.8 | |
| 0.00 | 1.17 | 0.00 | 0.61 | -4.81 | 20.12 | 16.77 | 256.02 | 0.2975 | -765.0 | -557.7 | |
| 0.00 | 0.63 | 0.00 | 0.33 | -9.71 | 19.72 | 16.37 | 240.62 | 0.3202 | -129.0 | -210.3 | |
| 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. | |