SDO HMI 2014-04-05 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.25 | 151.43 | 13.77 | 82.60 | 17.64 | 30.26 | 6.23 | 345.74 | 0.4205 | -289.8 | -352.2 | |
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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 |
| 1.67 | 125.58 | 0.91 | 68.56 | 17.37 | 31.30 | 7.26 | 343.22 | 0.4198 | -988.7 | -510.9 | |
| 1.85 | -1.00 | 1.01 | -1.00 | 17.53 | 31.27 | 7.24 | 343.39 | 0.4222 | -959.8 | 999999 | |
| 15.39 | -1.00 | 8.41 | -1.00 | 17.69 | 30.93 | 6.90 | 344.25 | 0.4231 | -1277.1 | 999999 | |
| 1.06 | -1.00 | 0.58 | -1.00 | 17.62 | 30.68 | 6.64 | 344.76 | 0.4210 | -1379.0 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.63 | 19.07 | 30.29 | 6.25 | 346.47 | 0.4416 | 639.0 | 479.5 | |
| 0.00 | 1.67 | 0.00 | 0.91 | 18.21 | 30.22 | 6.19 | 346.11 | 0.4282 | -642.0 | -632.8 | |
| 0.00 | 2.02 | 0.00 | 1.11 | 18.01 | 30.09 | 6.05 | 346.28 | 0.4246 | -789.0 | -655.7 | |
| 0.00 | 1.67 | 0.00 | 0.90 | 16.42 | 27.40 | 3.36 | 351.70 | 0.3914 | 872.0 | 681.1 | |
| 0.00 | 2.46 | 0.00 | 1.33 | 16.68 | 27.31 | 3.27 | 352.01 | 0.3954 | 785.0 | 684.3 | |
| 5.28 | 11.52 | 2.86 | 6.24 | 17.42 | 25.69 | 1.65 | 356.09 | 0.4046 | 1024.8 | 846.6 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 18.14 | 25.57 | 1.53 | 356.48 | 0.4160 | 827.0 | 684.2 | |
| 0.00 | 1.76 | 0.00 | 0.95 | 17.72 | 25.53 | 1.50 | 356.50 | 0.4091 | 783.0 | 589.2 | |
| 0.00 | 1.32 | 0.00 | 0.72 | 18.24 | 25.54 | 1.50 | 356.57 | 0.4175 | 619.0 | 562.7 | |
| 0.00 | 0.97 | 0.00 | 0.53 | 18.47 | 25.32 | 1.28 | 357.10 | 0.4210 | 786.0 | 705.9 | |
| 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. | |