SDO HMI 2014-12-01 03:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.54 | 0.00 | 10.83 | -5.10 | 94.51 | -4.17 | 159.15 | 0.1493 | 156.9 | 102.2 | |
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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 |
| 0.00 | 0.77 | 0.00 | 0.39 | -5.14 | 104.70 | 6.03 | 224.87 | 0.1489 | 750.0 | 517.8 | |
| 0.00 | 0.68 | 0.00 | 0.34 | -3.38 | 100.57 | 1.89 | 203.82 | 0.0818 | 329.0 | 500.4 | |
| 0.00 | 1.45 | 0.00 | 0.72 | -4.60 | 100.27 | 1.59 | 196.16 | 0.1001 | 936.0 | 651.1 | |
| 0.00 | 3.08 | 0.00 | 1.53 | -3.41 | 100.00 | 1.33 | 197.11 | 0.0789 | 803.0 | 700.3 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -4.48 | 100.00 | 1.33 | 193.85 | 0.0968 | 864.0 | 733.4 | |
| 0.00 | 0.94 | 0.00 | 0.47 | -1.46 | 99.71 | 1.03 | 203.70 | 0.0450 | 675.0 | 519.7 | |
| 0.00 | 1.37 | 0.00 | 0.68 | -2.25 | 99.38 | 0.70 | 192.62 | 0.0565 | 983.0 | 741.5 | |
| 0.00 | 2.91 | 0.00 | 1.48 | -10.03 | 92.26 | -6.42 | 149.82 | 0.2201 | 825.0 | 723.8 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -4.59 | 90.07 | -8.61 | 122.61 | 0.1779 | -881.0 | -653.0 | |
| 0.00 | 2.65 | 0.00 | 1.34 | -6.05 | 89.99 | -8.69 | 128.78 | 0.1936 | -729.0 | -425.4 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -5.60 | 89.60 | -9.07 | 125.74 | 0.1943 | -880.0 | -688.8 | |
| 0.00 | 2.31 | 0.00 | 1.17 | -5.46 | 89.39 | -9.28 | 124.51 | 0.1958 | -819.0 | -706.6 | |
| 0.00 | 1.71 | 0.00 | 0.86 | -3.11 | 89.10 | -9.58 | 112.73 | 0.1810 | -816.0 | -673.3 | |
| 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. | |