SDO HMI 2014-11-13 13:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.15 | 0.00 | 8.35 | -9.57 | 339.55 | 9.08 | 213.61 | 0.2780 | 161.9 | 62.4 | |
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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 | 1.20 | 0.00 | 0.65 | -6.40 | 352.06 | 21.59 | 246.34 | 0.4009 | 498.0 | 528.1 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -7.87 | 342.82 | 12.34 | 228.41 | 0.2844 | 953.0 | 822.8 | |
| 0.00 | 1.55 | 0.00 | 0.80 | -7.92 | 342.66 | 12.19 | 227.91 | 0.2832 | 886.0 | 686.1 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -10.67 | 341.62 | 11.15 | 218.83 | 0.3044 | 766.0 | 685.9 | |
| 0.00 | 0.95 | 0.00 | 0.49 | -9.78 | 340.88 | 10.41 | 218.86 | 0.2851 | 919.0 | 741.3 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -11.00 | 340.55 | 10.08 | 215.41 | 0.2979 | 704.0 | 549.5 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -10.84 | 340.43 | 9.95 | 215.38 | 0.2946 | 791.0 | 678.3 | |
| 0.00 | 1.89 | 0.00 | 0.97 | -9.87 | 337.41 | 6.94 | 208.10 | 0.2540 | -821.0 | -713.4 | |
| 0.00 | 1.20 | 0.00 | 0.62 | -12.62 | 336.53 | 6.06 | 200.91 | 0.2899 | -537.0 | -546.3 | |
| 0.00 | 1.89 | 0.00 | 0.96 | -8.18 | 334.58 | 4.11 | 200.05 | 0.2080 | -724.0 | -561.2 | |
| 0.00 | 1.20 | 0.00 | 0.61 | -9.21 | 334.35 | 3.88 | 197.49 | 0.2234 | -656.0 | -563.4 | |
| 0.00 | 1.38 | 0.00 | 0.71 | -11.32 | 334.16 | 3.69 | 194.30 | 0.2569 | -836.0 | -765.1 | |
| 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. | |