SDO HMI 2014-01-12 06:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.18 | 0.00 | 9.34 | -21.47 | 62.77 | 21.44 | 225.51 | 0.5065 | -363.5 | -265.7 | |
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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 |
| 0.00 | 1.19 | 0.00 | 0.78 | -13.66 | 81.36 | 40.03 | 253.92 | 0.6528 | -681.0 | -488.6 | |
| 0.00 | 1.02 | 0.00 | 0.65 | -12.54 | 79.74 | 38.40 | 255.26 | 0.6294 | -694.0 | -521.2 | |
| 0.00 | 1.36 | 0.00 | 0.83 | -19.01 | 74.56 | 33.23 | 242.82 | 0.5847 | 746.0 | 594.4 | |
| 0.00 | 1.19 | 0.00 | 0.72 | -19.30 | 74.11 | 32.78 | 242.09 | 0.5804 | 560.0 | 504.9 | |
| 0.00 | 1.02 | 0.00 | 0.61 | -18.32 | 73.49 | 32.16 | 243.35 | 0.5675 | 759.0 | 600.5 | |
| 0.00 | 1.02 | 0.00 | 0.60 | -26.02 | 66.45 | 25.12 | 225.34 | 0.5385 | 513.0 | 488.4 | |
| 0.00 | 1.02 | 0.00 | 0.56 | -17.61 | 63.12 | 21.79 | 236.31 | 0.4270 | -778.0 | -612.6 | |
| 0.00 | 0.94 | 0.00 | 0.51 | -17.13 | 62.70 | 21.36 | 236.83 | 0.4177 | -877.0 | -689.9 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -17.83 | 58.61 | 17.28 | 229.94 | 0.3711 | -939.0 | -760.4 | |
| 0.00 | 2.04 | 0.00 | 1.09 | -18.88 | 58.19 | 16.86 | 227.08 | 0.3765 | -893.0 | -749.1 | |
| 0.00 | 0.94 | 0.00 | 0.53 | -29.06 | 56.35 | 15.02 | 208.25 | 0.4805 | -456.0 | -376.8 | |
| 0.00 | 0.34 | 0.00 | 0.18 | -24.96 | 51.84 | 10.50 | 205.00 | 0.3928 | -387.0 | -481.5 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -30.86 | 52.04 | 10.71 | 199.57 | 0.4782 | -739.0 | -529.0 | |
| 0.00 | 0.94 | 0.00 | 0.52 | -32.17 | 39.10 | -2.23 | 175.97 | 0.4711 | -779.0 | -593.9 | |
| 0.00 | 1.45 | 0.00 | 0.83 | -34.26 | 34.28 | -7.05 | 168.54 | 0.5127 | -807.0 | -658.3 | |
| 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. | |