SDO HMI 2014-09-03 00:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.84 | 70.09 | 21.15 | 48.27 | -17.99 | 157.91 | -36.46 | 125.50 | 0.6961 | 214.1 | -84.7 | |
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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 |
| 9.39 | 25.39 | 6.29 | 17.03 | -17.74 | 159.72 | -34.65 | 126.51 | 0.6761 | 918.0 | 480.7 | |
| 6.53 | -1.00 | 4.37 | -1.00 | -17.42 | 159.52 | -34.85 | 125.96 | 0.6759 | 847.1 | 999999 | |
| 0.00 | 0.63 | 0.00 | 0.42 | -18.14 | 159.20 | -35.17 | 126.61 | 0.6842 | 408.0 | 391.9 | |
| 0.00 | 0.89 | 0.00 | 0.60 | -16.57 | 159.51 | -34.86 | 124.87 | 0.6701 | 614.0 | 542.7 | |
| 0.89 | 3.49 | 0.60 | 2.34 | -17.17 | 159.31 | -35.07 | 125.48 | 0.6764 | 705.9 | 484.0 | |
| 0.00 | 1.25 | 0.00 | 0.83 | -16.38 | 159.40 | -34.98 | 124.55 | 0.6700 | 726.0 | 614.1 | |
| 0.80 | 1.88 | 0.54 | 1.26 | -17.07 | 158.94 | -35.43 | 125.08 | 0.6795 | 553.2 | 451.6 | |
| 0.00 | 0.80 | 0.00 | 0.55 | -17.64 | 158.81 | -35.56 | 125.70 | 0.6848 | 450.0 | 339.9 | |
| 0.00 | 0.98 | 0.00 | 0.68 | -18.63 | 157.62 | -36.75 | 126.04 | 0.7035 | 393.0 | 247.1 | |
| 0.00 | 1.07 | 0.00 | 0.74 | -17.51 | 157.54 | -36.83 | 124.61 | 0.6969 | 522.0 | 420.8 | |
| 0.98 | 33.71 | 0.70 | 23.82 | -18.95 | 156.62 | -37.76 | 125.70 | 0.7155 | -673.3 | -565.9 | |
| 9.93 | -11.00 | 7.01 | -11.00 | -18.53 | 156.36 | -38.01 | 125.03 | 0.7154 | -818.0 | 999999 | |
| 0.89 | -11.00 | 0.63 | -11.00 | -18.16 | 156.46 | -37.92 | 124.65 | 0.7121 | -815.6 | 999999 | |
| 1.43 | -11.00 | 1.01 | -11.00 | -18.11 | 156.27 | -38.11 | 124.45 | 0.7136 | -771.2 | 999999 | |
| 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. | |