SDO HMI 2014-11-13 09:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.31 | 0.00 | 10.39 | -9.00 | 339.37 | 6.71 | 208.50 | 0.2490 | -20.8 | 29.6 | |
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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 | 1.55 | 0.00 | 0.80 | -5.12 | 345.43 | 12.77 | 237.39 | 0.2625 | 787.0 | 617.7 | |
| 0.00 | 2.07 | 0.00 | 1.06 | -5.08 | 344.21 | 11.55 | 234.87 | 0.2449 | 835.0 | 646.6 | |
| 0.00 | 1.98 | 0.00 | 1.01 | -7.89 | 342.71 | 10.05 | 222.47 | 0.2573 | 940.0 | 766.3 | |
| 0.00 | 1.46 | 0.00 | 0.76 | -10.73 | 341.57 | 8.91 | 212.64 | 0.2834 | 790.0 | 797.1 | |
| 0.00 | 1.46 | 0.00 | 0.75 | -9.75 | 340.87 | 8.21 | 212.50 | 0.2632 | 1101.0 | 880.3 | |
| 0.00 | 1.46 | 0.00 | 0.75 | -10.81 | 340.56 | 7.90 | 209.47 | 0.2759 | 848.0 | 718.7 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -9.45 | 337.23 | 4.58 | 200.00 | 0.2312 | -935.0 | -745.0 | |
| 0.00 | 3.36 | 0.00 | 1.71 | -9.84 | 337.24 | 4.58 | 199.44 | 0.2375 | -699.0 | -625.9 | |
| 0.00 | 1.12 | 0.00 | 0.57 | -10.05 | 337.06 | 4.40 | 198.44 | 0.2399 | -860.0 | -667.8 | |
| 0.00 | 0.86 | 0.00 | 0.44 | -9.38 | 336.27 | 3.61 | 196.10 | 0.2250 | -790.0 | -644.4 | |
| 0.00 | 1.46 | 0.00 | 0.75 | -11.27 | 334.71 | 2.05 | 188.09 | 0.2509 | -784.0 | -657.2 | |
| 0.00 | 1.46 | 0.00 | 0.74 | -9.19 | 334.22 | 1.56 | 187.24 | 0.2147 | -826.0 | -711.0 | |
| 0.00 | 0.69 | 0.00 | 0.35 | -11.32 | 333.84 | 1.18 | 184.64 | 0.2502 | -678.0 | -489.9 | |
| 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. | |