SDO HMI 2014-05-27 22:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.32 | 155.67 | 15.84 | 87.29 | -8.82 | 24.82 | -27.02 | 106.76 | 0.4706 | 689.3 | 414.6 | |
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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 |
| 21.02 | 136.93 | 11.73 | 76.40 | -8.82 | 25.37 | -26.48 | 107.02 | 0.4626 | 1238.2 | 456.1 | |
| 2.16 | -1.00 | 1.21 | -1.00 | -8.48 | 25.36 | -26.48 | 106.31 | 0.4614 | 876.4 | 999999 | |
| 1.44 | -1.00 | 0.81 | -1.00 | -9.00 | 24.94 | -26.90 | 107.17 | 0.4697 | 664.6 | 999999 | |
| 2.62 | -1.00 | 1.47 | -1.00 | -8.79 | 24.92 | -26.92 | 106.71 | 0.4691 | 790.1 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -7.74 | 24.56 | -27.29 | 104.36 | 0.4709 | 695.0 | 481.6 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -7.83 | 24.41 | -27.43 | 104.48 | 0.4733 | 805.0 | 581.2 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -7.98 | 24.23 | -27.62 | 104.71 | 0.4766 | 636.0 | 562.9 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -8.26 | 23.93 | -27.92 | 105.14 | 0.4819 | 465.0 | 499.3 | |
| 0.00 | 1.26 | 0.00 | 0.73 | -9.62 | 22.51 | -29.34 | 107.16 | 0.5075 | 810.0 | 747.1 | |
| 1.08 | 7.04 | 0.62 | 4.05 | -9.56 | 22.30 | -29.54 | 106.94 | 0.5103 | 912.4 | 711.3 | |
| 0.00 | 1.71 | 0.00 | 1.01 | -9.62 | 19.67 | -32.17 | 105.91 | 0.5480 | -841.0 | -682.7 | |
| 0.00 | 1.35 | 0.00 | 0.80 | -8.61 | 19.63 | -32.21 | 104.08 | 0.5455 | -696.0 | -627.4 | |
| 0.00 | 1.71 | 0.00 | 1.02 | -8.23 | 18.90 | -32.94 | 103.16 | 0.5548 | -659.0 | -446.5 | |
| 0.00 | 1.44 | 0.00 | 0.86 | -9.08 | 18.45 | -33.40 | 104.51 | 0.5636 | -738.0 | -579.3 | |
| 0.00 | 0.72 | 0.00 | 0.43 | -7.91 | 18.16 | -33.69 | 102.37 | 0.5646 | -516.0 | -424.6 | |
| 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. | |