SDO HMI 2014-01-14 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.61 | 20.02 | 0.87 | 10.85 | 17.19 | 27.34 | 9.61 | 336.52 | 0.4045 | -91.6 | -66.3 | |
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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 | 0.85 | 0.00 | 0.46 | 15.46 | 30.32 | 12.60 | 328.17 | 0.4003 | -664.0 | -495.6 | |
| 1.61 | 3.48 | 0.87 | 1.88 | 15.92 | 29.97 | 12.25 | 329.50 | 0.4037 | -878.0 | -694.6 | |
| 0.00 | 0.85 | 0.00 | 0.46 | 16.07 | 29.64 | 11.91 | 330.38 | 0.4031 | -618.0 | -518.4 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 16.00 | 28.82 | 11.09 | 332.00 | 0.3957 | -786.0 | -670.1 | |
| 0.00 | 1.10 | 0.00 | 0.60 | 17.01 | 28.60 | 10.87 | 333.66 | 0.4083 | -809.0 | -667.0 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 17.64 | 28.45 | 10.72 | 334.68 | 0.4163 | -774.0 | -634.7 | |
| 0.00 | 1.36 | 0.00 | 0.73 | 16.87 | 27.90 | 10.17 | 334.99 | 0.4016 | -814.0 | -697.7 | |
| 0.00 | 1.44 | 0.00 | 0.77 | 15.32 | 27.51 | 9.78 | 334.08 | 0.3765 | -790.0 | -689.0 | |
| 0.00 | 2.89 | 0.00 | 1.59 | 20.21 | 26.17 | 8.44 | 341.70 | 0.4405 | 785.0 | 616.7 | |
| 0.00 | 1.27 | 0.00 | 0.69 | 17.51 | 25.59 | 7.86 | 340.73 | 0.3970 | 942.0 | 743.1 | |
| 0.00 | 0.93 | 0.00 | 0.51 | 18.40 | 25.50 | 7.78 | 341.67 | 0.4101 | 711.0 | 552.3 | |
| 0.00 | 1.10 | 0.00 | 0.59 | 16.30 | 24.48 | 6.76 | 342.29 | 0.3729 | 784.0 | 661.3 | |
| 0.00 | 0.93 | 0.00 | 0.51 | 20.23 | 24.33 | 6.60 | 345.49 | 0.4325 | 769.0 | 628.9 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.15 | 22.13 | 4.41 | 348.14 | 0.3609 | 758.0 | 625.3 | |
| 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. | |