SDO HMI 2014-01-14 00:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.59 | 21.31 | 0.32 | 11.51 | 16.87 | 27.85 | 9.57 | 336.23 | 0.3986 | -352.9 | -300.9 | |
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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 |
| 0.59 | 3.14 | 0.32 | 1.70 | 15.92 | 29.93 | 11.65 | 330.71 | 0.3988 | -1005.6 | -819.6 | |
| 0.00 | 0.93 | 0.00 | 0.50 | 16.04 | 29.62 | 11.35 | 331.50 | 0.3981 | -678.0 | -563.5 | |
| 0.00 | 0.59 | 0.00 | 0.32 | 14.87 | 29.15 | 10.88 | 331.02 | 0.3781 | -815.0 | -675.6 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 16.06 | 28.75 | 10.48 | 333.40 | 0.3919 | -795.0 | -689.5 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 17.00 | 28.58 | 10.31 | 334.84 | 0.4043 | -799.0 | -684.8 | |
| 0.00 | 2.04 | 0.00 | 1.09 | 15.24 | 28.49 | 10.21 | 332.98 | 0.3783 | -739.0 | -559.0 | |
| 0.00 | 1.61 | 0.00 | 0.87 | 17.19 | 28.50 | 10.23 | 335.22 | 0.4064 | -812.0 | -637.9 | |
| 0.00 | 1.87 | 0.00 | 1.02 | 17.83 | 28.35 | 10.07 | 336.21 | 0.4146 | -729.0 | -603.4 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 16.90 | 27.76 | 9.49 | 336.50 | 0.3974 | -681.0 | -572.8 | |
| 0.00 | 1.53 | 0.00 | 0.82 | 15.35 | 27.50 | 9.23 | 335.39 | 0.3730 | -840.0 | -686.6 | |
| 0.00 | 2.04 | 0.00 | 1.12 | 20.21 | 26.21 | 7.93 | 342.72 | 0.4379 | 714.0 | 591.8 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 17.48 | 25.61 | 7.33 | 341.91 | 0.3937 | 872.0 | 784.6 | |
| 0.00 | 1.53 | 0.00 | 0.83 | 18.34 | 25.49 | 7.21 | 342.86 | 0.4063 | 746.0 | 576.8 | |
| 0.00 | 0.93 | 0.00 | 0.50 | 16.04 | 23.45 | 5.18 | 346.06 | 0.3617 | 830.0 | 645.6 | |
| 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. | |