SDO HMI 2014-11-12 06:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.23 | 0.00 | 8.87 | -9.03 | 339.69 | -7.79 | 154.00 | 0.2648 | 100.1 | 8.8 | |
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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 | 1.72 | 0.00 | 0.86 | -4.67 | 350.89 | 3.41 | 203.46 | 0.1495 | 946.0 | 584.2 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -4.49 | 350.86 | 3.38 | 203.76 | 0.1464 | 758.0 | 646.7 | |
| 0.00 | 0.86 | 0.00 | 0.43 | -4.96 | 343.62 | -3.86 | 154.63 | 0.1574 | 1048.0 | 890.2 | |
| 0.00 | 0.95 | 0.00 | 0.48 | -8.73 | 343.37 | -4.11 | 161.05 | 0.2191 | 990.0 | 808.8 | |
| 0.00 | 1.29 | 0.00 | 0.65 | -4.90 | 342.63 | -4.85 | 149.06 | 0.1645 | 1001.0 | 694.6 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -11.11 | 341.70 | -5.78 | 158.16 | 0.2669 | 833.0 | 550.4 | |
| 0.00 | 1.21 | 0.00 | 0.62 | -11.52 | 340.59 | -6.89 | 155.12 | 0.2805 | 723.0 | 576.1 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -10.41 | 337.02 | -10.46 | 142.66 | 0.2958 | -790.0 | -612.1 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -12.10 | 336.80 | -10.68 | 145.39 | 0.3205 | -810.0 | -706.6 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -12.28 | 336.79 | -10.69 | 145.71 | 0.3231 | -661.0 | -562.9 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -10.26 | 336.84 | -10.64 | 141.88 | 0.2956 | -885.0 | -669.0 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -9.71 | 336.67 | -10.80 | 140.25 | 0.2903 | -855.0 | -656.5 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -11.71 | 335.61 | -11.87 | 141.79 | 0.3271 | -849.0 | -636.3 | |
| 0.00 | 1.64 | 0.00 | 0.88 | -9.25 | 328.21 | -19.27 | 123.09 | 0.3904 | -48.0 | -35.7 | |
| 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. | |