SDO HMI 2014-12-06 22:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.36 | 0.00 | 8.67 | -14.16 | 37.28 | 14.92 | 225.20 | 0.3535 | -84.1 | -117.9 | |
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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 |
| 0.00 | 1.71 | 0.00 | 0.91 | -12.44 | 40.89 | 18.53 | 234.90 | 0.3811 | 650.0 | 628.2 | |
| 0.00 | 1.19 | 0.00 | 0.66 | -19.86 | 40.76 | 18.40 | 220.93 | 0.4551 | 694.0 | 548.2 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -15.18 | 39.25 | 16.89 | 226.68 | 0.3872 | 870.0 | 693.2 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -15.63 | 38.68 | 16.32 | 224.84 | 0.3856 | 857.0 | 748.9 | |
| 0.00 | 0.77 | 0.00 | 0.41 | -15.05 | 36.98 | 14.63 | 222.91 | 0.3598 | 790.0 | 557.7 | |
| 0.00 | 2.56 | 0.00 | 1.34 | -13.16 | 36.77 | 14.41 | 226.45 | 0.3359 | -710.0 | -399.4 | |
| 0.00 | 1.96 | 0.00 | 1.03 | -13.07 | 36.04 | 13.69 | 225.21 | 0.3263 | -1004.0 | -840.8 | |
| 0.00 | 1.96 | 0.00 | 1.03 | -13.37 | 35.84 | 13.49 | 224.12 | 0.3274 | -687.0 | -643.5 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -14.31 | 35.58 | 13.23 | 221.57 | 0.3356 | -958.0 | -702.7 | |
| 0.00 | 1.02 | 0.00 | 0.54 | -14.92 | 34.65 | 12.29 | 218.33 | 0.3332 | -609.0 | -527.8 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -10.77 | 33.71 | 11.36 | 225.57 | 0.2721 | -818.0 | -684.7 | |
| 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. | |