SDO HMI 2014-12-08 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.83 | 362.66 | 28.73 | 180.12 | -3.81 | 1.16 | -2.00 | 152.34 | 0.0752 | 1134.9 | 428.4 | |
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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 | 1.88 | 0.00 | 0.93 | -4.91 | 4.64 | 1.48 | 196.87 | 0.0891 | 868.0 | 609.2 | |
| 32.75 | 343.90 | 16.27 | 170.79 | -3.87 | 1.47 | -1.69 | 156.26 | 0.0733 | 1543.5 | 440.2 | |
| 0.00 | 1.02 | 0.00 | 0.51 | -2.45 | 1.12 | -2.04 | 139.80 | 0.0553 | 902.0 | 641.2 | |
| 22.26 | -2.00 | 11.06 | -2.00 | -3.60 | 0.85 | -2.31 | 147.10 | 0.0743 | 1463.0 | 999999 | |
| 1.11 | -2.00 | 0.55 | -2.00 | -3.84 | 0.82 | -2.34 | 148.43 | 0.0781 | 996.5 | 999999 | |
| 0.00 | 1.02 | 0.00 | 0.51 | -4.82 | 0.73 | -2.43 | 153.08 | 0.0938 | 784.0 | 618.0 | |
| 1.28 | 6.91 | 0.64 | 3.44 | -4.93 | 0.31 | -2.85 | 149.88 | 0.0991 | 940.0 | 612.6 | |
| 0.00 | 1.11 | 0.00 | 0.55 | -6.68 | 359.97 | -3.19 | 154.49 | 0.1288 | -776.0 | -612.0 | |
| 0.00 | 0.51 | 0.00 | 0.25 | -5.14 | 359.92 | -3.23 | 147.70 | 0.1057 | 726.0 | 734.0 | |
| 0.00 | 0.94 | 0.00 | 0.47 | -4.90 | 359.78 | -3.38 | 145.27 | 0.1036 | -791.0 | -521.6 | |
| 0.43 | 2.47 | 0.21 | 1.23 | -5.50 | 359.27 | -3.89 | 144.61 | 0.1172 | -1074.6 | -849.5 | |
| 0.00 | 1.88 | 0.00 | 0.93 | -3.10 | 358.48 | -4.68 | 123.22 | 0.0978 | 856.0 | 698.8 | |
| 0.00 | 1.02 | 0.00 | 0.51 | -4.72 | 357.99 | -5.16 | 132.31 | 0.1218 | -893.0 | -696.2 | |
| 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. | |