SDO HMI 2014-09-27 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 13.16 | 0.00 | 8.16 | -20.81 | 208.05 | -23.98 | 140.10 | 0.5971 | 224.2 | 139.6 | |
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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 |
| 0.00 | 1.15 | 0.00 | 0.65 | -17.45 | 215.26 | -16.77 | 145.93 | 0.4932 | 771.0 | 613.2 | |
| 0.00 | 1.94 | 0.00 | 1.13 | -18.80 | 213.66 | -18.37 | 145.09 | 0.5233 | -838.0 | -680.6 | |
| 0.00 | 0.62 | 0.00 | 0.39 | -26.49 | 211.29 | -20.74 | 149.73 | 0.6310 | 534.0 | 515.9 | |
| 0.00 | 1.24 | 0.00 | 0.79 | -25.81 | 210.63 | -21.40 | 148.33 | 0.6279 | 474.0 | 411.4 | |
| 0.00 | 0.71 | 0.00 | 0.46 | -25.89 | 208.19 | -23.84 | 145.64 | 0.6467 | 580.0 | 497.4 | |
| 0.00 | 0.88 | 0.00 | 0.58 | -25.88 | 206.94 | -25.09 | 144.30 | 0.6561 | 405.0 | 305.8 | |
| 0.00 | 0.71 | 0.00 | 0.41 | -13.50 | 208.75 | -23.28 | 131.39 | 0.5142 | 616.0 | 511.2 | |
| 0.00 | 1.59 | 0.00 | 1.07 | -27.48 | 206.07 | -25.96 | 144.94 | 0.6785 | 563.0 | 434.8 | |
| 0.00 | 2.03 | 0.00 | 1.20 | -15.02 | 207.22 | -24.81 | 131.79 | 0.5457 | 578.0 | 512.3 | |
| 0.00 | 1.32 | 0.00 | 0.82 | -15.33 | 201.86 | -30.17 | 126.78 | 0.6073 | -639.0 | -537.5 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -21.29 | 199.14 | -32.88 | 131.92 | 0.6822 | -578.0 | -411.8 | |
| 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. | |